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Diagnostics of the solar atmosphere by non-LTE inverse method: Line of Ba II λ 455.403 nm. 2016 ;32(1):33-42.
. 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.
. 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.
. Diagnostics of horizontal velocities field in the solar atmosphere: line Ba II λ 455.403 nm. 2016 ;32(3):63-74.
. Peculiarities of the excitation and propagation of the gravity waves in the solar photosphere. Russian. 2012 ;28(3):73-80.
. Reflection of acoustic waves in the real solar atmosphere. Russian. 2010 ;26(2):50-58.
. Features of convection in the atmosphere layers of the solar facula. Ukrainian. 2019 ;35(6):18-33.
. Structure of the solar photosphere convection on subgranulation scales. 2008 ;24(2):99-109.
. Solar faculae: microturbulence as an indicator of inclined magnetic fields. Ukrainian. 2020 ;36(4):3-18.
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