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Diagnostics of the solar atmosphere by inverse methods: hydrogen absorption lines. 2005 ;21(6):461-470.
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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.
. Properties of convective motions in the upper solar atmosphere. I. Russian. 2010 ;26(5):26-40.
. Reflection of acoustic waves in the real solar atmosphere. Russian. 2010 ;26(2):50-58.
. The effect of magnetic field on fine structure of convective motions in the solar atmosphere. Russian. 2012 ;28(4):3-14.
. "Solar" oscillator strength scale and determination of the LTE silicon abundance in the solar atmosphere. Russian. 2012 ;28(2):3-21.
. Solar spectrum of silicon and diagnostics of the solar atmosphere. Russian. 2012 ;28(1):45-58.
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