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1Shchukina NG, 1Vasilieva IE. Oscillator strengths of selected Fe II lines in the range λλ 300-400 n. Russian. 2013 ;29(2):3-21.
1Shchukina NG, 1Kostyk RI. Results of observations of wave motions in the Solar facula. Ukrainian. 2022 ;38(1):71-89.
1Shchukina NG, 2Trujillo B, 1Vasilieva IE, 3Frantseva KV. Center-to-limb variation of the continuum intensity and linear polarization of stars with transiting exoplanets. Russian. 2017 ;33(4):29-50.
1Shchukina NG, 1Sukhorukov AV. "Solar" oscillator strength scale and determination of the LTE silicon abundance in the solar atmosphere. Russian. 2012 ;28(2):3-21.
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.
1Shchukina NG, 1Sukhorukov AV. NLTE formation of the silicon spectrum: silicon abundance in three-dimensional model of the solar atmosphere. Russian. 2013 ;29(1):26-49.
1Sheminova VA. Fourier analysis of spectra of solar-type stars. Russian. 2017 ;33(5):27-48.
1Sheminova VA. Temperature stratification of the Arcturus atmosphere. Russian. 2013 ;29(4):31-60.
1Sheminova VA. The line asymmetry in the spectra of the Sun and solar-type stars. Ukrainian. 2020 ;36(6):65-87.
1Sheminova VA. Convective lineshifts in the spectra of the Sun and solar-type stars. Ukrainian. 2022 ;38(2):39-62.

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