Nonchaotic and globally synchronized short-term climatic variations and their origin

  • I. V. SerykhEmail author
  • D. M. Sonechkin
Original Paper


Careful computations of atmospheric power spectra are done. These computations reveal that these spectra are continuous in the range of timescales from 2 days to 1 year, and so they confirm that weather variations are chaotic; however, the continuity of a part of the atmospheric power spectra, corresponding to the periods from 2 years to one decade is questioned. This part is prominent by the existence of several narrow bands of increased spectral density centered at the subharmonics 2:1, 3:1, and 4:1 of the Chandler wobble in the Earth’s pole motion (~ 1.2 years); the superharmonics 1:2, 1:3, and 1:4 of the Luni-Solar nutation of the Earth’s rotation axis (~ 18.6 years) as well as the superharmonics 1:2, 1:3, and 1:4 of the 11-year cycle of the Sun spots. The existence of similar bands in the El Niño–Southern Oscillation (ENSO) power spectra was recognized many years ago; however, it turns out that the above spectral bands also are seen in spectra of the atmospheric characteristics outside of tropics. Moreover, the respective climatic variations are globally synchronized. The synchronization takes place because the above-mentioned external periodicities must influence short-term climatic variations everywhere on the Earth. It is very probable that the periods of the external periodicities indicated are incommensurable with each other. Therefore, if these periodicities actually influence short-term climatic variations, they would have to do it discordantly. As a result, no resonances can exist which could make the affected climatic variations to be chaotic. A linear dependence of logarithms of serial numbers of the spectral bands on logarithms of the band magnitudes as well as a linear decrease of the accumulated sum of the squared autocorrelations of the respective atmospheric characteristics confirm that the dynamics of the interannual to decadal climatic variations are not chaotic.


Supplementary material

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© Springer-Verlag GmbH Austria, part of Springer Nature 2019

Authors and Affiliations

  1. 1.Shirshov Institute of OceanologyRussian Academy of SciencesMoscowRussia

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