Skip to main content

Thank you for visiting nature.com. You are using a browser version with limited support for CSS. To obtain the best experience, we recommend you use a more up to date browser (or turn off compatibility mode in Internet Explorer). In the meantime, to ensure continued support, we are displaying the site without styles and JavaScript.

  • Letter
  • Published:

Variations of the Sun's radius and temperature due to magnetic buoyancy

Abstract

LIVINGSTON1 has recently measured a decrease in the surface temperature of the Sun coincident with increased solar activity. He interpreted the temperature drop as implying a corresponding reduction in luminosity. I point out here that surface cooling could also be due to a radial expansion of the Sun, with no attendant reduction in luminosity. There is a plausible physical mechanism for such an expansion; namely, variations in magnetic buoyancy due to variations in the magnetic flux in the convection zone over the solar cycle.

This is a preview of subscription content, access via your institution

Access options

Buy this article

Prices may be subject to local taxes which are calculated during checkout

Similar content being viewed by others

References

  1. Livingston, W. C. Nature 272, 340–341 (1978).

    Article  ADS  Google Scholar 

  2. Parker, E. N. Astrophys. J. 121, 491–507 (1955).

    Article  ADS  Google Scholar 

  3. Jensen, E. Ann. Astrophys. 18, 127–140 (1955).

    ADS  Google Scholar 

  4. Weiss, N. O. Mon. Not. R. astr. Soc. 128, 225–235 (1964).

    Article  ADS  Google Scholar 

  5. Harvey, J. W. in Highlights of Astronomy (ed. Müller, E.) Vol. 4, 223–239 (Reidel, Dordrecht, 1977).

    Book  Google Scholar 

  6. Galloway, D. J., Proctor, M. R. E. & Weiss, N. O. Nature 266, 686–689 (1977).

    Article  ADS  Google Scholar 

  7. Goldberg, L. in The Sun (ed. Kuiper, G. P.) 1–35 (University of Chicago Press, 1953).

    Google Scholar 

  8. Gething, P. J. D. Mon. Not. R. astr. Soc. 115, 558–570 (1955).

    Article  ADS  Google Scholar 

  9. Wittmann, A. Solar Phys. 29, 333–340 (1973).

    Article  ADS  CAS  Google Scholar 

  10. Auwers, A. Astr. Nachr. 128, 367 (1891).

    ADS  Google Scholar 

  11. Cullen, R. T. Mon. Not. R. astr. Soc. 86, 344–349 (1926).

    Article  ADS  Google Scholar 

  12. Giannuzzi, M. A. Contr. Sci. Oss. Roma, No. 211 (1955).

  13. Meyermann, B. Astr. Nachr. 279, 45–46 (1950).

    Article  ADS  Google Scholar 

  14. Hill, H. A., Stebbins, R. T. & Oleson, J. R. Astrophys. J. 200, 484–498 (1975).

    Article  ADS  Google Scholar 

  15. Dicke, R. H. & Goldenberg, H. M. Phys. Rev. Lett. 18, 313–316 (1967).

    Article  ADS  Google Scholar 

  16. Hill, H. A. & Stebbins, R. T. Astrophys. J. 200, 471–483 (1975).

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

THOMAS, J. Variations of the Sun's radius and temperature due to magnetic buoyancy. Nature 280, 662–663 (1979). https://doi.org/10.1038/280662a0

Download citation

  • Received:

  • Accepted:

  • Issue Date:

  • DOI: https://doi.org/10.1038/280662a0

This article is cited by

Comments

By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.

Search

Quick links

Nature Briefing

Sign up for the Nature Briefing newsletter — what matters in science, free to your inbox daily.

Get the most important science stories of the day, free in your inbox. Sign up for Nature Briefing