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On the heliosphere characteristics important for galactic cosmic rays in the phase of minimum solar activity

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Abstract

Various heliospheric parameters important for the behavior of cosmic rays, i.e., the solar wind velocity, heliospheric magnetic field, and heliospheric current sheet during epochs of the minimum of solar cycles 20–24 are discussed. Main features and regularities of the behavior of these parameters and their interrelations are considered.

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Authors and Affiliations

  1. Lebedev Physical Institute, Russian Academy of Sciences, Leninskii pr. 53, Moscow, 119991, Russia

    M. B. Krainev

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  1. M. B. Krainev
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Correspondence to M. B. Krainev.

Additional information

Original Russian Text © M.B. Krainev, 2012, published in Kratkie Soobshcheniya po Fizike, 2012, Vol. 39, No. 6, pp. 13–20.

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Krainev, M.B. On the heliosphere characteristics important for galactic cosmic rays in the phase of minimum solar activity. Bull. Lebedev Phys. Inst. 39, 170–174 (2012). https://doi.org/10.3103/S1068335612060024

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  • DOI: https://doi.org/10.3103/S1068335612060024

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