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Solar Physics

, Volume 205, Issue 1, pp 165–175 | Cite as

Time Evolution of low-Frequency Periodicities in Cosmic ray Intensity

  • K. Kudela
  • J. Rybák
  • A. Antalová
  • M. Storini
Article

Abstract

The long-time series of daily means of cosmic-ray intensity observed by four neutron monitors at different cutoff rigidities (Calgary, Climax, Lomnický Štít and Huancayo/Haleakala) were analyzed by means of the wavelet transform method in the period range ∼ 60 to ∼ 1000 days. The contributions of the time evolution of three quasi-periodic cosmic-ray signals (∼ 150 d, ∼ 1.3 yr and ∼ 1.7 yr) to the global one are obtained. While the ∼ 1.7-yr quasi-periodicity, the most remarkable one in the studied interval, strongly contributes to the cosmic ray intensity profile of solar cycle 21 (particularly in 1982), the ∼ 1.3-yr one, which is better correlated with the same periodicity of the interplanetary magnetic field strength, is present as a characteristic feature for the decreasing phases of the cycles 20 and 22. Transitions between these quasi-periodicities are seen in the wavelet power spectra plots. Obtained results support the claimed difference in the solar activity evolution during odd and even solar activity cycles.

Keywords

Time Evolution Power Spectrum Solar Activity Solar Cycle Magnetic Field Strength 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Kluwer Academic Publishers 2002

Authors and Affiliations

  • K. Kudela
    • 1
  • J. Rybák
    • 2
  • A. Antalová
    • 1
  • M. Storini
    • 3
  1. 1.IEP/SASKošiceSlovak Republic
  2. 2.Astronomical Institute/SASTatranská LomnicaSlovak Republic
  3. 3.Area di Ricerca Roma-Tor VergataIFSI/CNR

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