Skip to main content

A topological model of the solar magnetic field reversals

  • Part III Solar magnetism and large-scale flows
  • Conference paper
  • First Online:
The Sun and Cool Stars: activity, magnetism, dynamos

Part of the book series: Lecture Notes in Physics ((LNP,volume 380))

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Institutional subscriptions

References

  • Benevolenskaya, E.E. and Makarov, V.I.: 1990, Soln. Dann. No 5, 75

    Google Scholar 

  • Hoyng, P.: 1990 in Solar Photosphere: Structure, Convection and Magnetc Fields, ed. Stenflo, O.J., IAU Symp. No 138, p. 359

    Google Scholar 

  • Kleeorin, N.I. and Ruzmaikin, A.A: 1988, Preprint IZMIRAN, No 7(833), p. 3

    Google Scholar 

  • Makarov, V.I., Tavastsherna, K.S. and Petrova, N.S.: 1985, Soln. Dann. No 6, 69

    Google Scholar 

  • Parker, E.N.: 1979, Cosmical Magnetic Fields, Oxford University Press.

    Google Scholar 

  • Wang, J.W., Nash, A.G. and Sheeley, N.R.,Jr.: 1989, Astrophys. J. 347, 529

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Editor information

I. Tuominen D. Moss G. Rüdiger

Rights and permissions

Reprints and permissions

Copyright information

© 1991 Springer-Verlag

About this paper

Cite this paper

Benevolenskaya, E.E. (1991). A topological model of the solar magnetic field reversals. In: Tuominen, I., Moss, D., Rüdiger, G. (eds) The Sun and Cool Stars: activity, magnetism, dynamos. Lecture Notes in Physics, vol 380. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-53955-7_132

Download citation

  • DOI: https://doi.org/10.1007/3-540-53955-7_132

  • Published:

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-53955-1

  • Online ISBN: 978-3-540-46483-9

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics