Hostname: page-component-848d4c4894-m9kch Total loading time: 0 Render date: 2024-06-08T11:28:21.624Z Has data issue: false hasContentIssue false
  • English
  • Français

Stellar Dynamo Characteristics

Published online by Cambridge University Press:  30 March 2016

N.O. Weiss
N.O. Weiss*
Affiliation:
Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge CB3 9EW, England

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Recent discoveries have shown that magnetic activity is typical of cool stars with deep convective zones and magnetic cycles are found in slowly rotating stars like the sun. The current state of hydromagnetic dynamo theory is reviewed, and simplified models are used in an attempt to isolate the dominant nonlinear processes in stellar dynamos.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 7: Highlights of Astronomy. As presented at the XIXth General Assembly of the IAU, 1985 , 1986 , pp. 385 - 392
Copyright
Copyright © Reidel 1986

References

Baliunas, S.L. and 11 others: 1985, Astrophys. J. 294, 310.CrossRefGoogle Scholar
Baliunas, S.L. and Vaughan, A.H.: 1985, Ann. Rev. Astron. Astrophys. 23, 379.Google Scholar
van Ballegooijen, A.: 1982, Astron. Astrophys. 115, 99.Google Scholar
Borra, E.F., Edwards, G. and Mayor, M.: 1984, Astrophys. J. 284, 211.CrossRefGoogle Scholar
Cowling, T.G.: 1981, Ann. Rev. Astron. Astrophys. 19, 115.Google Scholar
Duvall, T.L. and 5 others: 1984, Nature 310, 22.Google Scholar
Eddy, J.A.: 1976, Science 286, 1189.CrossRefGoogle Scholar
Giampapa, M.S.: 1983, in “Solar and Stellar Magnetic Fields”, ed. Stenflo, J.O., Reidel, Dordrecht, p. 187.Google Scholar
Giampapa, M.S. and Rosner, R.: 1984, Astrophys. J. 286, L19.Google Scholar
Gilman, P.A.: 1979, Astrophys. J. 231, 284.CrossRefGoogle Scholar
Gilman, P.A.: 1983, Astrophys. J. Suppl. Ser. 53, 243.Google Scholar
Gilman, P.A. and Howard, R.: 1984, Astrophys. J. 285, 385.CrossRefGoogle Scholar
Glatzmaier, G.A.: 1985a, Astrophys. J. 291, 300.CrossRefGoogle Scholar
Glatzmaier, G.A.: 1985b, Geophys. Astrophys. Fluid Dyn. 31, 137.Google Scholar
Gray, D.F.: 1984, Astrophys. J. 277, 640.Google Scholar
Hughes, D.W.: 1985a, Geophys. Astrophys. Fluid Dyn. 32, 273.CrossRefGoogle Scholar
Hughes, D.W.: 1985b, Geophys. Astrophys. Fluid Dyn. (in press).Google Scholar
Ivanova, T.S. and Ruzmaikin, A.A.: 1977, Astron. Zh. 54, 846; Sov. Astron. 21, 479.Google Scholar
Jones, C.A.: 1984, in “Hydromagnetics of the Sun”, ed. Guyenne, T. ESA SP-220, Noordwijk, p.91.Google Scholar
Kleeorin, N.I., Ruzmaikin, A.A. and Sokoloff, D.D.: 1983, Astrophys. Space Sci. 95, 131.CrossRefGoogle Scholar
LaBonte, B.J. and Howard, R.F.: 1982, Solar Phys. 75, 161.Google Scholar
Langford, W.F.: 1983, in “Nonlinear Dynamics and Turbulence”, ed. Barenblatt, G.I. Iooss, G. and Joseph, D.D., Pitman, London, p.215.Google Scholar
Lockwood, G.W. and 6 others: 1984, Publ. Astron. Soc. Pac. 96, 714.CrossRefGoogle Scholar
Marcy, G.W.: 1984, Astrophys. J. 276, 286.CrossRefGoogle Scholar
Noyes, R.W., Hartmann, L.W., Baliunas, S.L., Duncan, D.K. and Vaughan, A.H.: 1984a, Astrophys. J. 279, 763.CrossRefGoogle Scholar
Noyes, R.W., Weiss, N.O. and Vaughan, A.H.: 1984b, Astrophys. J. 287, 769.Google Scholar
Pallavicini, R. and 5 others: 1981, Astrophys. J. 248, 279.Google Scholar
Parker, E.N.: 1979, “Cosmical Magnetic Fields”, Clarendon Press, Oxford.Google Scholar
Robinson, R.D., Worden, P.W. and Harvey, J.W.: 1980, Astrophys. J. 236, L155.CrossRefGoogle Scholar
Rosner, R. and Weiss, N.O.: 1985, Nature 317, 790.Google Scholar
Ruzmaikin, A.A.: 1984, in “Hydromagnetics of the Sun”, ed. Guyenne, T., ESA SP-220, Noordwijk, p.85.Google Scholar
Schmitt, J. and Rosner, R.: 1983, Astrophys. J. 266, 901.Google Scholar
Schüssler, M.: 1981, Astron. Astrophys. 94, 755.Google Scholar
Schüssler, M.: 1983, in “Solar and Stellar Magnetic Fields”, ed. Stenflo, J.O., Reidel, Dordrecht, p.213.Google Scholar
Snodgrass, H.B. and Howard, R. : 1985, Solar Phys. 95, 221.CrossRefGoogle Scholar
Soderblom, D.R.: 1985, Astrophys. J. (submitted).Google Scholar
Spiegel, E.A. and Weiss, N.O.: 1980, Nature 287, 616.Google Scholar
Spörer, G.: 1889, Nova Acta Ksl. Leop. – Carol. Deutschen Akad. Naturforscher 53, 272.Google Scholar
Stuiver, M. : 1980, Nature 286, 868.Google Scholar
Stuiver, M. and Quay, P.D.: 1980, Science 207, 11.Google Scholar
Stauffer, J.R., Hartmann, L.W., Burnham, J.N. and Jones, B.F.: 1985, Astrophys. J. 289, 247.Google Scholar
Stauffer, J.R., Hartmann, L.W., Soderblom, D.R. and Burnham, N.: 1984, Astrophys. J. 280, 202.Google Scholar
Vaiana, G.S. and 15 others: 1981, Astrophys. J. 245, 163.Google Scholar
Vaughan, A.H. and Preston, G. : 1980, Publ. Astron. Soc. Pac. 92, 385.Google Scholar
Vaughan, A.H. and 6 others: 1981, Astrophys. J. 250, 276.Google Scholar
Weiss, N.O.: 1983, in “Stellar and Planetary Magnetism”, ed. Soward, A.M., Gordon $ Breach, London, p.115.Google Scholar
Weiss, N.O.: 1985, J. Stat. Phys. 39, 477.Google Scholar
Weiss, N.O., Jones, C.A. and Cattaneo, F.: 1984, Geophys. Astrophys. Fluid Dyn. 30, 305.CrossRefGoogle Scholar
Wilson, O.C.: 1978, Astrophys. J. 226, 279.Google Scholar
Yoshimura, H.: 1978, Astrophys. J. 220, 692.Google Scholar
Yoshimura, H.: 1981, Astrophys. J. 247, 1102.CrossRefGoogle Scholar
Zel’dovich, Ya. B., Ruzmaikin, A.A. and Sokoloff, D.D.: 1983, “Magnetic Fields in Astrophysics”, Gordon & Breach, London.Google Scholar