Hostname: page-component-848d4c4894-4rdrl Total loading time: 0 Render date: 2024-06-29T04:59:08.293Z Has data issue: false hasContentIssue false
  • English
  • Français

Observations Relating to Stellar Activity, Magnetism and Dynamos

Published online by Cambridge University Press:  12 April 2016

C. Jordan
C. Jordan*
Affiliation:
Department of Theoretical Physics, University of Oxford, 1 Keble Road, Oxford 0X1 3NP, UK

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.

Dynamo theory can in principle be tested by comparing its predictions with a variety of types of solar and stellar observations. The progress apparent from papers presented at this Colloquium is summarized, and areas where further observations would be of particular value are stressed.

Type
Concluding summaries
Information
International Astronomical Union Colloquium , Volume 130: The Sun and Cool Stars: activity, magnetism, dynamos , 1991 , pp. 509 - 514
Copyright
Copyright © Springer-Verlag 1991

References

Chapman, G.A.: 1988, Editor, Adv. in Space Res. Vol. 8, No. 7.Google Scholar
Howard, R.H., LaBonte, B.J.: 1980, Astrophys. J. Letts. 239, L33.Google Scholar
Howard, R.H., Gilman, P.A., Gilman, P.I.: 1984, Astrophys. J. 283, 373.Google Scholar
Jordan, C.: 1990, In Proc. of Heidelberg Conf. on Mechanisms of Coronal Heating, June, 1990. In Press.Google Scholar
Jordan, C., Ayres, T.R., Brown, A., Linsky, J.L., Simon, T.: 1987, Mon. Not. R. astr. Soc. 225, 903.Google Scholar
Mein, P., Ribes, E.: 1990, Astron. Astrophys. 227, 577.Google Scholar
Montesinos, B., Jordan, C.: 1988, in A Decade of UV Astronomy with IUE, ESA SP-281, Vol. 1, 283.Google Scholar
Noyes, R.W., Hartmann, L.W., Baliunas, S.L., Duncan, D.K., Vaughan, A.H.: 1984, Astrophys. J. 279, 763.Google Scholar
Parker, E.N.: 1975, Astrophys. J. 108, 205.CrossRefGoogle Scholar
Parker, E.N.: 1987, Sol. Phys. 110, 11.Google Scholar
Reeves, E.M.: 1976, Sol. Phys. 46, 53.Google Scholar
Rutten, R.G.M.: 1987, Astron. Astrophys. 177, 131.Google Scholar
Saar, S.H.: 1990, in Solar Photosphere: Structure, Convection and Magnetic Fields, Proc. IAU Symp. 138, ed. Stenflo, J.O., Kluwer, Dordrecht, p. 427.Google Scholar
Schrijver, C.J.: 1987, Astron. Astrophys. 172, 111.Google Scholar
Schrijver, C.J., Cote, J., Zwaan, C., Saar, S.H.: 1989, Astrophys. J. 337, 964.Google Scholar
Schrijver, C.J., Zwaan, C., Maxson, C.W., Noyes, R.W.: 1985, Astr. Astrophys. 149, 123.Google Scholar
Sitnik, G.F., Kozlova, L.M., Divlikeev, M.I., Porfiryeva, G.A.: 1986, Soviet Solar Data, No. 12, 67.Google Scholar
Skumanich, A., Lean, J.L., White, O.R., Livingston, W.C.: 1984, Astrophys. J. 282, 776.Google Scholar
Snodgrass, H.B.: 1986, Astrophys. J. Letts. 316, L91.Google Scholar
Tuominen, J.: 1945, The Observatory 66, 160.Google Scholar