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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.
1Kostogryz NM. Raman scattering in Uranus's spectrum with regard to nonisothermal atmosphere. 2006 ;22(4):254-259.
1Kostyk RI. What mechanisms allow the 5-minute oscillations in the active regions of the solar surface to penetrate from the photosphere into the chromosphere?. Russian. 2015 ;31(4):45-53.
1Kostyk RI. Effect of wave motions in the active region of the solar surface on convection. Russian. 2018 ;34(2):46-54.
1Kostyk RI, 1Shchukina NG, 2Kobanov NI, 2Pulyaev VA. The influence of magnetic field on the propagation of 5-min oscillations in the solar atmosphere: the phase shifts. Russian. 2014 ;30(1):61-69.
1Kostyk RI. What are solar faculae?. Russian. 2013 ;29(1):50-57.

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