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.

Unusual activity of the Sun during recent decades compared to the previous 11,000 years

Abstract

Direct observations of sunspot numbers are available for the past four centuries1,2, but longer time series are required, for example, for the identification of a possible solar influence on climate and for testing models of the solar dynamo. Here we report a reconstruction of the sunspot number covering the past 11,400 years, based on dendrochronologically dated radiocarbon concentrations. We combine physics-based models for each of the processes connecting the radiocarbon concentration with sunspot number. According to our reconstruction, the level of solar activity during the past 70 years is exceptional, and the previous period of equally high activity occurred more than 8,000 years ago. We find that during the past 11,400 years the Sun spent only of the order of 10% of the time at a similarly high level of magnetic activity and almost all of the earlier high-activity periods were shorter than the present episode. Although the rarity of the current episode of high average sunspot numbers may indicate that the Sun has contributed to the unusual climate change during the twentieth century, we point out that solar variability is unlikely to have been the dominant cause of the strong warming during the past three decades3.

Access options

Rent or Buy article

Get time limited or full article access on ReadCube.

from$8.99

All prices are NET prices.

Figure 1: Atmospheric radiocarbon level Δ14C (expressed as deviation, in ‰, from the ad 1950 standard level15) derived from mostly decadal samples of absolutely dated tree-ring chronologies (INTCAL98 data set)16.
Figure 2: Comparison between directly measured sunspot number (SN) and SN reconstructed from different cosmogenic isotopes.
Figure 3: Reconstructed sunspot number and its uncertainty for the whole interval of time considered.
Figure 4: Distribution of the duration of episodes of high solar activity and the probability that the current episode will reach a given duration.

References

  1. 1

    Hoyt, D. V. & Schatten, K. H. Group sunspot numbers: A new solar activity reconstruction. Sol. Phys. 179, 189–219 (1998)

    ADS  Article  Google Scholar 

  2. 2

    Eddy, J. A. The Maunder minimum. Science 192, 1189–1202 (1976)

    ADS  CAS  Article  Google Scholar 

  3. 3

    Solanki, S. K. & Krivova, N. Can solar variability explain global warming since 1970? J. Geophys. Res. 108, doi: 10.1029/2002JA009753 (2003)

  4. 4

    Stuiver, M. & Braziunas, T. F. Atmospheric 14C and century-scale solar oscillations. Nature 338, 405–408 (1989)

    ADS  CAS  Article  Google Scholar 

  5. 5

    Stuiver, M. & Braziunas, T. F. Sun, ocean, climate and atmospheric 14CO2: an evaluation of causal and spectral relationships. Holocene 3, 289–305 (1993)

    ADS  Article  Google Scholar 

  6. 6

    Damon, P. E. & Sonett, C. P. in The Sun in Time (eds Sonnet, C. P., Giampapa, M. S. & Matthews, M. S.) 360–388 (Univ. Arizona, Tucson, 1991)

    Google Scholar 

  7. 7

    Beer, J. et al. Use of 10Be in polar ice to trace the 11-year cycle of solar activity. Nature 347, 164–166 (1990)

    ADS  CAS  Article  Google Scholar 

  8. 8

    Beer, J. Long-term indirect indices of solar variability. Space Sci. Rev. 94, 53–66 (2000)

    ADS  CAS  Article  Google Scholar 

  9. 9

    Solanki, S. K., Schüssler, M. & Fligge, M. Evolution of the Sun's large-scale magnetic field since the Maunder minimum. Nature 408, 445–447 (2000)

    ADS  CAS  Article  Google Scholar 

  10. 10

    Solanki, S. K., Schüssler, M. & Fligge, M. Secular variation of the Sun's magnetic flux. Astron. Astrophys. 383, 706–712 (2002)

    ADS  Article  Google Scholar 

  11. 11

    Usoskin, I. G., Alanko, K., Mursula, K. & Kovaltsov, G. A. Heliospheric modulation strength during the neutron monitor era. Sol. Phys. 207, 389–399 (2002)

    ADS  CAS  Article  Google Scholar 

  12. 12

    Usoskin, I. G., Mursula, K., Solanki, S. K., Schüssler, M. & Kovaltsov, G. A. A physical reconstruction of cosmic ray intensity since 1610. J. Geophys. Res. 107, doi:10.1029/2002JA009343 (2002)

  13. 13

    Usoskin, I. G., Mursula, K., Solanki, S. K., Schüssler, M. & Alanko, K. Reconstruction of solar activity for the last millenium using 10Be data. Astron. Astrophys. 413, 745–751 (2004)

    ADS  Article  Google Scholar 

  14. 14

    Usoskin, I. G., Solanki, S. K., Schüssler, M., Mursula, K. & Alanko, K. A millenium scale sunspot number reconstruction: evidence for an unusually active Sun since the 1940s. Phys. Rev. Lett. 91, 211101 (2003)

    ADS  Article  Google Scholar 

  15. 15

    Stuiver, M. & Pollach, P. Discussion: reporting of 14C data. Radiocarbon 19, 355–363 (1977)

    Article  Google Scholar 

  16. 16

    Stuiver, M. et al. INTCAL98 Radiocarbon age calibration. Radiocarbon 40, 1041–1083 (1998)

    CAS  Article  Google Scholar 

  17. 17

    Broecker, W. S. An unstable superconveyor. Nature 367, 414–415 (1994)

    ADS  Article  Google Scholar 

  18. 18

    Bond, G. et al. Persistent solar influence on North Atlantic surface circulation during the Holocene. Science 294, 2130–2136 (2001)

    ADS  CAS  Article  Google Scholar 

  19. 19

    Muscheler, R., Beer, J. & Kromer, B. Solar Variability as an Input to the Earth's Environment 305–316 (ESA SP-535, European Space Agency, Noordwijk, 2003)

    Google Scholar 

  20. 20

    Bard, E., Raisbeck, G. M., Yiou, F. & Jouzel, J. Solar modulation of cosmogenic nuclide production over the last millennium: comparison between 14C and 10Be records. Earth Planet. Sci. Lett. 150, 453–462 (1997)

    ADS  CAS  Article  Google Scholar 

  21. 21

    Usoskin, I. G. & Kromer, B. Reconstruction of the 14C production rate from measured relative abundance. Radiocarbon (in the press)

  22. 22

    Suess, H. E. Radiocarbon content in modern wood. Science 122, 415–417 (1955)

    ADS  CAS  Article  Google Scholar 

  23. 23

    Elsasser, W., Ney, E. P. & Winckler, J. R. Cosmic-ray intensity and geomagnetism. Nature 178, 1226–1227 (1956)

    ADS  Article  Google Scholar 

  24. 24

    Castagnoli, G. & Lal, D. Solar modulation effects in terrestrial production of carbon-14. Radiocarbon 22, 133–158 (1980)

    CAS  Article  Google Scholar 

  25. 25

    Hongre, L., Hulot, G. & Khokhlov, A. An analysis of the geomagnetic field over the past 2000 years. Phys. Earth Planet. Inter. 106, 311–335 (1998)

    ADS  Article  Google Scholar 

  26. 26

    Yang, S., Odah, H. & Shaw, J. Variations in the geomagnetic dipole moment over the last 12000 years. Geophys. J. Int. 140, 158–162 (2000)

    ADS  Article  Google Scholar 

Download references

Author information

Affiliations

Authors

Corresponding author

Correspondence to S. K. Solanki.

Ethics declarations

Competing interests

The authors declare that they have no competing financial interests.

Supplementary information

Supplementary Information

Estimates of errors of sunspot number reconstruction from 14C data. (PDF 171 kb)

Rights and permissions

Reprints and Permissions

About this article

Cite this article

Solanki, S., Usoskin, I., Kromer, B. et al. Unusual activity of the Sun during recent decades compared to the previous 11,000 years. Nature 431, 1084–1087 (2004). https://doi.org/10.1038/nature02995

Download citation

Further reading

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