¹Shchukina NG, ¹Kostyk RI. Results of observations of wave motions in the Solar facula. Ukrainian. 2022 ;38(1):71-89.

¹Shchukina NG, ¹Kostyk RI. Diagnostics of the velocity field of the quiet Sun using the lambda-meter method: the Si I λ 1082.7 nm line. Ukrainian. 2020 ;36(1):3-23.

¹Stodilka MI, ²Kostyk RI. Solar faculae: microturbulence as an indicator of inclined magnetic fields. Ukrainian. 2020 ;36(4):3-18.

¹Stodilka MI, ¹Prysiazhnyi AI, ²Kostyk RI. Features of convection in the atmosphere layers of the solar facula. Ukrainian. 2019 ;35(6):18-33.

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

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, 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.

¹Kozak LV, ²Kostyk RI, ³Cheremnykh OK. Two turbulent regimes on the Sun. Russian. 2013 ;29(2):22-29.

¹Kostyk RI. What are solar faculae?. Russian. 2013 ;29(1):50-57.