Two-component photospheric models of a solar flare of 2N/M2 class
. Two-component photospheric models of a solar flare of 2N/M2 class. Russian. 2014 ;30(2):58-69.
Solar Physics
The influence of magnetic field on the propagation of 5-min oscillations in the solar atmosphere: the phase shifts
. 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.
Pre-flare changes of the solar photosphere using THEMIS observations data
. Pre-flare changes of the solar photosphere using THEMIS observations data. Russian. 2014 ;30(1):50-60.
Some problems of asymmetry of coronal spectral lines
. Some problems of asymmetry of coronal spectral lines. Russian. 2015 ;31(5):49-60.
Power of the energy of the 11-year solar cycle and its dependence on the duration of the solar cycle
. Power of the energy of the 11-year solar cycle and its dependence on the duration of the solar cycle. Russian. 2015 ;31(4):54-60.
What mechanisms allow the 5-minute oscillations in the active regions of the solar surface to penetrate from the photosphere into the chromosphere?
Some asymmetry in distribution of Hα flares on the solar disk during the 21th cycle
. Some asymmetry in distribution of Hα flares on the solar disk during the 21th cycle. Russian. 2015 ;31(3):54-62.
The structure of the solar photospheric convection on granular and mesogranular scales
. The structure of the solar photospheric convection on granular and mesogranular scales. Russian. 2015 ;31(2):21-33.
On the small-scale alpha-squared effect in the convection zone of the Sun
. On the small-scale alpha-squared effect in the convection zone of the Sun. Russian. 2015 ;31(2):3-20.
Robust method for determination of magnetic field strength in solar photosphere
. Robust method for determination of magnetic field strength in solar photosphere. Ukrainian. 2018 ;34(6):3-21.