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] . On one type of three-wave interaction of low-frequency waves in magnetoactive plasma of the solar atmosphere. Russian. 2014 ;30(3):58-70.
. Peculiarities of solar photospheric convection at granular, mesogranular and supergranular scales. Ukrainian. 2014 ;30(4):23-37.
. Physical conditions in the chromosphere of a solar two-ribbon flare, accompanied by a surge. II. Russian. 2014 ;30(6):14-26.
. On the possibility of the development of longitudinal wave instabilities on the background of the small-scale Bernstein turbulence in preflare chromosphere of a solar active region. Russian. 2014 ;30(5):39-55.
. Pre-flare changes of the solar photosphere using THEMIS observations data. Russian. 2014 ;30(1):50-60.
. Spatial variations of Stokes profiles of magnetoactive Fe I lines. Russian. 2014 ;30(6):3-13.
. NLTE formation of the silicon spectrum: silicon abundance in three-dimensional model of the solar atmosphere. Russian. 2013 ;29(1):26-49.
. Oscillator strengths of selected Fe II lines in the range λλ 300-400 n. Russian. 2013 ;29(2):3-21.
. Physical conditions in the chromosphere of a solar two-ribbon flare accompanied by a surge. I. Russian. 2013 ;29(4):18-30.
. A prediction of amplitude for solar cycle 24 using dynamics of activity near the cycle minimum. Russian. 2013 ;29(1):58-67.