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What mechanisms allow the 5-minute oscillations in the active regions of the solar surface to penetrate from the photosphere into the chromosphere?. Russian. 2015 ;31(4):45-53.
. What are solar faculae?. Russian. 2013 ;29(1):50-57.
. Two turbulent regimes on the Sun. Russian. 2013 ;29(2):22-29.
. The influence of magnetic field on the propagation of 5-min oscillations in the solar atmosphere: the phase shifts. Russian. 2014 ;30(1):61-69.
. Features of convection in the atmosphere layers of the solar facula. Ukrainian. 2019 ;35(6):18-33.
. Effect of wave motions in the active region of the solar surface on convection. Russian. 2018 ;34(2):46-54.
. Diagnostics of the velocity field of the quiet Sun using the lambda-meter method: the Si I λ 1082.7 nm line. Ukrainian. 2020 ;36(1):3-23.
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