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Quasiperiodic Variations of Solar Activity and Cosmic Rays

  • Astronomy, Astrophysics, and Cosmology
  • Published:
Moscow University Physics Bulletin Aims and scope

Abstract

Quasiperiodic variations of various manifestations of solar activity, parameters of the interplanetary medium, and the flux of galactic cosmic rays (GCRs) are studied using the data of stratospheric sounding and measurements with neutron monitors. Groups of spectral components with periods of ~2, 1.3, and ~1 year are identified in the range of periods shorter than 5 years. Particular attention is paid to quasi-2-year GCR variations that are induced by similar variations of the mean magnetic field of the Sun and are integral to the processes of solar activity.

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Authors and Affiliations

  1. Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, 119991, Russia

    V. P. Okhlopkov

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  1. V. P. Okhlopkov
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Correspondence to V. P. Okhlopkov.

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Original Russian Text © V.P. Okhlopkov, 2018, published in Vestnik Moskovskogo Universiteta, Seriya 3: Fizika, Astronomiya, 2018, No. 2, pp. 102–112.

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Okhlopkov, V.P. Quasiperiodic Variations of Solar Activity and Cosmic Rays. Moscow Univ. Phys. 73, 223–233 (2018). https://doi.org/10.3103/S002713491802011X

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  • DOI: https://doi.org/10.3103/S002713491802011X

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