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Robust method for determination of magnetic field strength in solar photosphere. Ukrainian. 2018 ;34(6):3-21.
. Oscillator strengths of selected Fe II lines in the range λλ 300-400 n. Russian. 2013 ;29(2):3-21.
. NLTE formation of the silicon spectrum: silicon abundance in three-dimensional model of the solar atmosphere. Russian. 2013 ;29(1):26-49.
. Spatial variations of Stokes profiles of magnetoactive Fe I lines. Russian. 2014 ;30(6):3-13.
. Features of convection in the atmosphere layers of the solar facula. Ukrainian. 2019 ;35(6):18-33.
. Diagnostics of photospheric jets of the quiet Sun atmosphere. Ukrainian. 2019 ;35(5):48-84.
. Spatial structure of gravity waves in the solar photosphere. Russian. 2013 ;29(4):3-17.
. Solar faculae: microturbulence as an indicator of inclined magnetic fields. Ukrainian. 2020 ;36(4):3-18.
. History of sun spot research and forecast of the maximum of solar cycle 25. Ukrainian. 2021 ;37(4):60-78.
. The influence of solar activity on seasonal variation of the methane absorption in Saturn's atmosphere. Russian. 2015 ;31(3):38-53.
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