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Diagnostics of horizontal velocities field in the solar atmosphere: line Ba II λ 455.403 nm. 2016 ;32(3):63-74.
. Reflection of acoustic waves in the real solar atmosphere. Russian. 2010 ;26(2):50-58.
. Diagnostics of the solar atmosphere by non-LTE inverse method: Line of Ba II λ 455.403 nm. 2016 ;32(1):33-42.
. "Solar" oscillator strength scale and determination of the LTE silicon abundance in the solar atmosphere. Russian. 2012 ;28(2):3-21.
. NLTE formation of the Ba II λ 455.4 nm resonance line in the solar atmosphere. 2008 ;24(3):198-215.
. Stability of magnetic configurations of solar atmosphere in temperature anisotropy conditions. Russian. 2008 ;24(5):360-369.
. To the nonlinear interaction of low-frequency kinetic plasma waves in the pre-flare atmosphere of solar active region. Ukrainian. 2022 ;38(3):47-64.
. The effect of magnetic field on fine structure of convective motions in the solar atmosphere. Russian. 2012 ;28(4):3-14.
. Properties of convective motions in the upper solar atmosphere. I. Russian. 2010 ;26(5):26-40.
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