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:

The effect of flares on total solar irradiance

Abstract

Flares are powerful bursts of energy released by relatively poorly understood processes that take place in the atmospheres of stars1. However, although solar flares, from our own Sun, are the most energetic events in the solar system, in comparison to the total output of the Sun they are barely noticeable2,3. Consequently, the total amount of radiant energy they generate is not precisely known, and their potential contribution to variations in the total solar irradiance4 incident on the Earth has so far been overlooked. In this work, we identify a measurable signal from relatively moderate solar flares in total solar irradiance data. We find that the total energy radiated by flares exceeds by two orders of magnitude the flare energy radiated in the soft-X-ray domain only, indicating a major contribution in the visible domain. These results have implications for our understanding of solar-flare activity and the variability of our star.

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

Figure 1: Detection of flares in the TSI through superposed-epoch analysis.
Figure 2: Averaged TSI variations during flares of smaller amplitudes.
Figure 3: Total energy radiated by solar flares versus the energy radiated in X-rays.

Similar content being viewed by others

References

  1. Haisch, B., Strong, K. T. & Rodono, M. Flares on the sun and other stars. Annu. Rev. Astron. Astrophys. 29, 257–324 (1991).

    Article  ADS  Google Scholar 

  2. Hudson, H. S. & Willson, R. C. Upper limits on the total radiant energy of solar flares. Sol. Phys. 86, 123–130 (1983).

    Article  ADS  Google Scholar 

  3. Woods, T. N. et al. Solar irradiance variability during the October 2003 solar storm period. Geophys. Res. Lett. 31, L10802 (2004).

    Article  ADS  Google Scholar 

  4. Fröhlich, C. & Lean, J. Solar radiative output and its variability: Evidence and mechanisms. Astron. Astrophys. Rev. 12, 273–320 (2004).

    Article  ADS  Google Scholar 

  5. Carrington, R. C. Description of a singular appearance seen in the sun on September 1. Mon. Not. R. Astron. Soc. 20, 13–15 (1859).

    Article  ADS  Google Scholar 

  6. Neidig, D. F. The importance of solar white-light flares. Sol. Phys. 121, 261–269 (1989).

    Article  ADS  Google Scholar 

  7. Woods, T. N., Kopp, G. & Chamberlin, P. C. Contributions of the solar ultraviolet irradiance to the total solar irradiance during large flares. J. Geophys. Res. 111, A10S14 (2006).

    Article  ADS  Google Scholar 

  8. Johnsen, H., Pécseli, H. L. & Trulsen, J. Conditional eddies in plasma turbulence. Phys. Fluids 30, 2239–2254 (1987).

    Article  ADS  Google Scholar 

  9. Frohlich, C. et al. First results from VIRGO, the experiment for helioseismology and solar irradiance monitoring on SOHO. Sol. Phys. 170, 1–25 (1997).

    Article  ADS  MathSciNet  Google Scholar 

  10. Emslie, A. G. et al. Refinements to flare energy estimates: A followup to ‘Energy partition in two solar flare/CME events’. J. Geophys. Res. 110, 11103 (2005).

    Article  Google Scholar 

Download references

Acknowledgements

This work has received funding from the European Community’s Seventh Framework Programme (FP7/2007-2013) under the grant agreement No 218816 (SOTERIA project, www.soteria-space.eu). J-F.H., T.D.d.W. and M.K. also acknowledge financial support from the French–Belgian partnership program ‘Tournesol’.

Author information

Authors and Affiliations

Authors

Contributions

S.D., S.M., W.S. and J-F.H. were involved in the design of the study. T.D.d.W. was involved in the analysis of the data. M.K. analysed the data and drafted the manuscript. All authors discussed the results and commented on the manuscript.

Corresponding author

Correspondence to Matthieu Kretzschmar.

Ethics declarations

Competing interests

The authors declare no competing financial interests.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Kretzschmar, M., de Wit, T., Schmutz, W. et al. The effect of flares on total solar irradiance. Nature Phys 6, 690–692 (2010). https://doi.org/10.1038/nphys1741

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1038/nphys1741

This article is cited by

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