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A modernization of the analysis method for vertical structure of aerosol component in giant planet atmospheres. Russian. 2013 ;29(6):53-67.
. 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.
. A procedure of determination of troposphere delays in the network of active reference stations ZAKPOS/UA-EUPOS. Russian. 2013 ;29(4):73-0.
. On reality of families of periodic and long-periodic comets of Uranus. Russian. 2013 ;29(2):50-61.
. A sample of Wolf-Rayet galaxies from the Sloan Digital Sky Survey. Russian. 2013 ;29(3):48-63.
. Shadow mechanism and opposition effect of light for atmosphereless celestial bodies. Russian. 2013 ;29(5):36-48.
. A slitless spectrograph for small telescopes: initial results. Russian. 2013 ;29(3):64-0.
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