Анон. NLTE formation of the Ba II λ 455.4 nm resonance line in the solar atmosphere. 2008 ;24(3):198-215.

Анон. Fe I line pairs of different magnetic sensitivity. 2009 ;25(6):482-489.

Анон. NLTE formation of the solar silicon spectrum. Silicon abundance in one-dimensional models of the solar atmosphere. Russian. 2012 ;28(4):27-48.

Анон. "Solar" oscillator strength scale and determination of the LTE silicon abundance in the solar atmosphere. Russian. 2012 ;28(2):3-21.

Анон. Solar spectrum of silicon and diagnostics of the solar atmosphere. Russian. 2012 ;28(1):45-58.

Анон. NLTE formation of the silicon spectrum: silicon abundance in three-dimensional model of the solar atmosphere. Russian. 2013 ;29(1):26-49.

Анон. Oscillator strengths of selected Fe II lines in the range λλ 300-400 n. Russian. 2013 ;29(2):3-21.

Анон. 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.

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

Анон. Robust method for determination of magnetic field strength in solar photosphere. Ukrainian. 2018 ;34(6):3-21.