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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.
. Spatial structure of gravity waves in the solar photosphere. Russian. 2013 ;29(4):3-17.
. Two turbulent regimes on the Sun. Russian. 2013 ;29(2):22-29.
. What are solar faculae?. Russian. 2013 ;29(1):50-57.
. On cyclicity of solar magnetic fields during cycles 21-23. Russian. 2012 ;28(3):62-72.
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