NLTE formation of the silicon spectrum: silicon abundance in three-dimensional model of the solar atmosphere 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.
Physical conditions in the chromosphere of a solar two-ribbon flare, accompanied by a surge. II 1Baranovskii EA, 2Kondrashova NN, 2Pasechnik MN, 1Tarashchuk VP. Physical conditions in the chromosphere of a solar two-ribbon flare, accompanied by a surge. II. Russian. 2014 ;30(6):14-26.
Spatial variations of Stokes profiles of magnetoactive Fe I lines 1Stodilka MI. Spatial variations of Stokes profiles of magnetoactive Fe I lines. Russian. 2014 ;30(6):3-13.
On the possibility of the development of longitudinal wave instabilities on the background of the small-scale Bernstein turbulence in preflare chromosphere of a solar active region 1Kryshtal AN, 1Voitsekhovska AD, 1Gerasimenko SV, 2Sidorenko MV. On the possibility of the development of longitudinal wave instabilities on the background of the small-scale Bernstein turbulence in preflare chromosphere of a solar active region. Russian. 2014 ;30(5):39-55.
Peculiarities of solar photospheric convection at granular, mesogranular and supergranular scales 1Baran OA, 1Stodilka MI. Peculiarities of solar photospheric convection at granular, mesogranular and supergranular scales. Ukrainian. 2014 ;30(4):23-37.
Plasma motions in the solar loop of the emerging magnetic flux 1Pasechnik MN. Plasma motions in the solar loop of the emerging magnetic flux. Russian. 2014 ;30(4):3-22.
On one type of three-wave interaction of low-frequency waves in magnetoactive plasma of the solar atmosphere 1Kryshtal AN, 1Gerasimenko SV, 1Voitsekhovska AD, 2Cheremnykh OK. On one type of three-wave interaction of low-frequency waves in magnetoactive plasma of the solar atmosphere. Russian. 2014 ;30(3):58-70.
Two-component photospheric models of a solar flare of 2N/M2 class 1Andriiets OS, 2Kondrashova NN, 1Kurochka EV. Two-component photospheric models of a solar flare of 2N/M2 class. Russian. 2014 ;30(2):58-69.
The influence of magnetic field on the propagation of 5-min oscillations in the solar atmosphere: the phase shifts 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.