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1Neomenko R, 2Novosyadlyi B. Dynamics of expansion of the Universe in the models with non-minimally coupled dark energy. 2016 ;32(4):3-22.
1Petrenko BA, 1Kozak LV. Dynamics of magnetic structures during the magnetospheric substorm. Ukrainian. 2020 ;36(5):55-63.
1Pishkalo MI, 1Leiko UM. Dynamics of near-polar magnetic field of the Sun at the maximum of solar cycle 24. 2016 ;32(2):37-47.
1Fedorov YI, 1Shakhov BA, 1Kolesnyk YL. Dynamics of solar cosmic ray energetic spectra during the solar flare on January 20, 2005. Russian. 2015 ;31(4):3-20.
1Kryvodubskyj VN. Dynamo-parameters of the convection zone of the Sun. Ukrainian. 2006 ;22(1):3-28.
E
Lozitsky VG, Efimenko VM. Early forecast of maximum of 25th cycle of Solar activity. 2023 ;39(1):65-71.
Miller NO, Prudnikova EY. Early latitude observations at the Pulkovo Observatory. Russian. 2011 ;27(1):40-52.
1Kostik RI. The effect of magnetic field on fine structure of convective motions in the solar atmosphere. Russian. 2012 ;28(4):3-14.
1Kolesnyk YL, 1Klyuyeva AI, 1Shakhov BA, 1Fedorov YI. The effect of solar wind high-speed streams on the galactic cosmic rays intensity. 2016 ;32(6):3-19.
1Kolesnyk YL, 1Shakhov BA. The effect of the heliopause and a standing termination shock on the propagation of galactic cosmic rays in heliosphere stationary model. Russian. 2012 ;28(6):3-16.

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