Solar Physics
Solar faculae: microturbulence as an indicator of inclined magnetic fields
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
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
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
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.
. Features of convection in the atmosphere layers of the solar facula
Features of convection in the atmosphere layers of the solar facula. Ukrainian. 2019 ;35(6):18-33.
. Diagnostics of photospheric jets of the quiet Sun atmosphere
Diagnostics of photospheric jets of the quiet Sun atmosphere. Ukrainian. 2019 ;35(5):48-84.
. On the role of MHD turbulence in the decrease of electric conductivity of plasma in the active magnetic area of the Sun
Low-frequency kinetic waves in plasmas of magnetic loops at the early stage of flare process in active region
Low-frequency kinetic waves in plasmas of magnetic loops at the early stage of flare process in active region. Russian. 2019 ;35(3):3-33.
. Fraunhofer lines in the transition from the center to the limb of the solar disk
Fraunhofer lines in the transition from the center to the limb of the solar disk. Russian. 2019 ;35(2):50-64.
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