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Peculiarities of the excitation and propagation of the gravity waves in the solar photosphere. Russian. 2012 ;28(3):73-80.
. The influence of small scale magnetic fields on profiles of magnetically sensitive λ 525.02 nm and λ 1564.85 nm Fe I lines in the quiet solar photosphere. 2011 ;27(4):3-23.
. Spatial structure of gravity waves in the solar photosphere. Russian. 2013 ;29(4):3-17.
. Spatial variations of Stokes profiles of magnetoactive Fe I lines. Russian. 2014 ;30(6):3-13.
. Diagnostics of the solar atmosphere by non-LTE inverse method: Line of Ba II λ 455.403 nm. 2016 ;32(1):33-42.
. Global isothermal oscillations in the solar photosphere. Russian. 2011 ;27(3):28-39.
. Solar faculae: microturbulence as an indicator of inclined magnetic fields. Ukrainian. 2020 ;36(4):3-18.
. NLTE formation of the solar silicon spectrum. Silicon abundance in one-dimensional models of the solar atmosphere. Russian. 2012 ;28(4):27-48.
. Solar spectrum of silicon and diagnostics of the solar atmosphere. Russian. 2012 ;28(1):45-58.
. On photometric observations of geostationary satellites near equinox dates. Russian. 2014 ;30(2):70-76.
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