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Hysteresis of indices of solar and ionospheric activity during 11-year cycles

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Abstract

The effects of hysteresis, which is a manifestation of ambiguous relationships between different solar activity indices during the rising and declining phases of solar cycles, are analyzed. The paper addresses the indices characterizing radiation from the solar photosphere, chromosphere, and corona, and the ionospheric indices. The 21st, 22nd, and 23rd solar cycles, which significantly differ from each other in amplitude, exhibit different extents of hysteresis.

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Authors and Affiliations

  1. Sternberg Astronomical Institute, Moscow State University, Moscow, 119991, Russia

    E. A. Bruevich & G. V. Yakunina

  2. Federov Institute of Applied Geophysics, Moscow, 129128, Russia

    T. V. Kazachevskaya, V. V. Katyushina & A. A. Nusinov

Authors
  1. E. A. Bruevich
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  2. T. V. Kazachevskaya
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  3. V. V. Katyushina
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  4. A. A. Nusinov
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  5. G. V. Yakunina
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Correspondence to E. A. Bruevich.

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Bruevich, E.A., Kazachevskaya, T.V., Katyushina, V.V. et al. Hysteresis of indices of solar and ionospheric activity during 11-year cycles. Geomagn. Aeron. 56, 1075–1081 (2016). https://doi.org/10.1134/S001679321608003X

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  • DOI: https://doi.org/10.1134/S001679321608003X

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