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On the Reproduction of the Solar Activity Variations in the Range 2–40 Months in the Interplanetary Medium

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Abstract

We compare the quasi-biennial variations and Rieger-type variations (on a timescale of less than 1 year) in solar activity, interplanetary magnetic field, and galactic cosmic-ray flux modulation. We show that, in comparison with the 11-year cycle, the quasi-biennial variations are less suppressed in the interplanetary medium than on the Sun. Although the Rieger-type variations are adjacent in frequency to the quasi-biennial variations, they differ noticeably from them in the degree of reproduction in the interplanetary medium and the influence on the cosmic-ray modulation.

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ACKNOWLEDGMENTS

We are grateful to our colleagues from the laboratory of solar physics and cosmic rays named after S.N. Vernov (the Dolgoprudny scientific station of the Lebedev Physical Institute of the Russian Academy of Sciences), who created homogeneous series of data on the charged-particle fluxes in the Earth’s atmosphere through their long-term work, and the researchers that provide free access to the data on the Internet: https://wwwbis.sidc.be/silso/datafiles (Rz); https://omniweb.gsfc.nasa.gov/form/dx1.html (IMF data); and http://cosrays.izmiran.ru (NM data, Moscow).

Funding

This work was performed within budgetary funding.

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Authors and Affiliations

  1. Lebedev Physical Institute, Russian Academy of Sciences, 119991, Moscow, Russia

    G. A. Bazilevskaya, M. S. Kalinin, M. B. Krainev, V. S. Makhmutov, A. K. Svirzhevskaya, N. S. Svirzhevsky & Yu. I. Stozhkov

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  1. G. A. Bazilevskaya
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  2. M. S. Kalinin
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  3. M. B. Krainev
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  4. V. S. Makhmutov
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  5. A. K. Svirzhevskaya
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  6. N. S. Svirzhevsky
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  7. Yu. I. Stozhkov
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Correspondence to G. A. Bazilevskaya.

Additional information

A paper for the special issue of JETP devoted to the centenary of A.E. Chudakov

Translated by V. Astakhov

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Bazilevskaya, G.A., Kalinin, M.S., Krainev, M.B. et al. On the Reproduction of the Solar Activity Variations in the Range 2–40 Months in the Interplanetary Medium. J. Exp. Theor. Phys. 134, 479–486 (2022). https://doi.org/10.1134/S1063776122040021

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  • DOI: https://doi.org/10.1134/S1063776122040021

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