¹Kostyk RI. Effect of wave motions in the active region of the solar surface on convection. Russian. 2018 ;34(2):46-54.

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.

¹Kostik RI. Solar faculae and floccules: spectropolarimetric and filter observations in Fe I, Ba II, and Ca II lines. 2024 ;40(1):65-74.

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.

¹Korsun AA. Determination of secular polar motion from astronomical observations. The priority of O. Ya. Orlov. 2016 ;32(2):74-80.

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.