A prediction of amplitude for solar cycle 24 using dynamics of activity near the cycle minimum
. A prediction of amplitude for solar cycle 24 using dynamics of activity near the cycle minimum. Russian. 2013 ;29(1):58-67.
Solar Physics
What are solar faculae?
. What are solar faculae?. Russian. 2013 ;29(1):50-57.
NLTE formation of the silicon spectrum: silicon abundance in three-dimensional model of the solar atmosphere
. 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
. 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
. 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
Peculiarities of solar photospheric convection at granular, mesogranular and supergranular scales
. 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
. 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
. 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
. Two-component photospheric models of a solar flare of 2N/M2 class. Russian. 2014 ;30(2):58-69.