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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.
. 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.
. 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.
. Center-to-limb variation of the continuum intensity and linear polarization of stars with transiting exoplanets. Russian. 2017 ;33(4):29-50.
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