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Solar Physics

, Volume 289, Issue 12, pp 4701–4709 | Cite as

Cosmogenic Isotope Variability During the Maunder Minimum: Normal 11-year Cycles Are Expected

  • S. V. Poluianov
  • I. G. Usoskin
  • G. A. Kovaltsov
Article

Abstract

The amplitude of the 11-year cycle measured in the cosmogenic isotope 10Be during the Maunder Minimum is comparable to that during the recent epoch of high solar activity. Because of the virtual absence of the cyclic variability of sunspot activity during the Maunder Minimum this seemingly contradicts an intuitive expectation that lower activity would result in smaller solar-cycle variations in cosmogenic radio-isotope data, or in none, leading to confusing and misleading conclusions. It is shown here that large 11-year solar cycles in cosmogenic data observed during periods of suppressed sunspot activity do not necessarily imply strong heliospheric fields. Normal-amplitude cycles in the cosmogenic radio-isotopes observed during the Maunder Minimum are consistent with theoretical expectations because of the nonlinear relation between solar activity and isotope production. Thus, cosmogenic-isotope data provide a good tool to study solar-cycle variability even during grand minima of solar activity.

Keywords

Cosmic rays Maunder minimum Solar cycle 

Notes

Acknowledgements

G.K. acknowledges partial support from the Program No. 22 of Presidium RAS. Support by the Academy of Finland to the ReSoLVE Center of Excellence (project no. 272157) is acknowledged.

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Copyright information

© Springer Science+Business Media Dordrecht 2014

Authors and Affiliations

  • S. V. Poluianov
    • 1
  • I. G. Usoskin
    • 1
    • 3
  • G. A. Kovaltsov
    • 2
  1. 1.Department of PhysicsUniversity of OuluOuluFinland
  2. 2.Ioffe Physical-Technical InstituteSt. PetersburgRussia
  3. 3.Sodankylä Geophysical Observatory (Oulu Unit)University of OuluOuluFinland

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