λ17.1 nm Fe IX Line in the radiation spectrum of slow magneto-acoustic waves propagating in the solar crown

¹Mamedov SG, Aliyeva ZF, Alisheva KI. λ17.1 nm Fe IX Line in the radiation spectrum of slow magneto-acoustic waves propagating in the solar crown. Ukrainian. 2021 ;37(6):49-61.

History of sun spot research and forecast of the maximum of solar cycle 25

¹Vasilieva IE, ²Pishkalo MI. History of sun spot research and forecast of the maximum of solar cycle 25. Ukrainian. 2021 ;37(4):60-78.

Development of a solar circular flare М6.4 according to observations in the Нα line

¹Chornogor SN, ¹Kondrashova NN. Development of a solar circular flare М6.4 according to observations in the Нα line. 2021 ;37(2):41-56.

Prediction of solar cycle 25: maximum in the N- and S-hemispheres

¹Pishkalo MI. Prediction of solar cycle 25: maximum in the N- and S-hemispheres. 2021 ;37(1):48-56.

Generation by global migratory flow of variable magnetic field of the Sun

¹Loginov AA, ²Kryvodubskyj VN, ¹Cheremnykh OK. Generation by global migratory flow of variable magnetic field of the Sun. 2021 ;37(1):30-47.

Spectral study of active region site with Ellerman bomb and Нα-ejections. chromosphere. Ellerman bomb

¹Pasechnik MN. Spectral study of active region site with Ellerman bomb and Нα-ejections. chromosphere. Ellerman bomb. 2021 ;37(1):3-29.

Solar faculae: microturbulence as an indicator of inclined magnetic fields

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

Morphology of the flare-productive active region NOAA 9087

¹Chornogor SN, ¹Kondrashova NN. Morphology of the flare-productive active region NOAA 9087. Ukrainian. 2020 ;36(3):69-90.

Generation of the radial magnetic field of the Sun by global hydrodynamic flows

¹Loginov AA, ²Kryvodubskyj VN, ¹Cheremnykh OK. Generation of the radial magnetic field of the Sun by global hydrodynamic flows. Ukrainian. 2020 ;36(2):20-33.

Diagnostics of the velocity field of the quiet Sun using the lambda-meter method: the Si I λ 1082.7 nm line

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.

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