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1Kornienko YV, Skuratovsk, ii SI. The accumulation of Fourier-component phases in case of an object observation through a turbulent atmosphere. II. Russian. 2012 ;28(2):45-58.
Korniienko YV, Skuratovsk, ii SI. Fourier-components phase accumulation in the observation of an object through a turbulent atmosphere. I. Russian. 2011 ;27(6):52-63.
1Korsun AA. Determination of secular polar motion from astronomical observations. The priority of O. Ya. Orlov. 2016 ;32(2):74-80.
1Koshmak IO, 1Melekh BY. Modelling of H II region emission with bubble-like structure inside. Ukrainian. 2013 ;29(6):3-19.
1Koshmak IO, 1Melekh BY. Modelling of H II region radiation surrounding the starburst knot taking into account the structures evolution formed by superwind. Ukrainian. 2017 ;33(2):3-23.
1Koshmak IO, 1Melekh BY. Multicomponent simulation of emission of low-metallicity H II regions. Ukrainian. 2014 ;30(2):26-47.
1Kostik RI. Solar faculae and floccules: spectropolarimetric and filter observations in Fe I, Ba II, and Ca II lines. 2024 ;40(1):65-74.
1Kostik RI. Properties of convective motions in the upper solar atmosphere. I. Russian. 2010 ;26(5):26-40.
1Kostik RI. Some properties of convective motions in the upper solar atmosphere. II. Russian. 2011 ;27(4):24-34.
1Kostik RI. The effect of magnetic field on fine structure of convective motions in the solar atmosphere. Russian. 2012 ;28(4):3-14.

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