Reflection of acoustic waves in the real solar atmosphere 1Stodilka MI. Reflection of acoustic waves in the real solar atmosphere. Russian. 2010 ;26(2):50-58.
Generation of low-frequency magnetic disturbances in coronal loops by proton and electron beams 1Malovichko PP. Generation of low-frequency magnetic disturbances in coronal loops by proton and electron beams. Russian. 2010 ;26(2):36-49.
Line-of-sight veloсities of photospheric matter motion in a solar flare with ejection 1Kondrashova NN, 1Pasechnik MN. Line-of-sight veloсities of photospheric matter motion in a solar flare with ejection. Russian. 2010 ;26(1):57-73.
Line-of-sight veloсity field in low atmosphere of an active region during a solar flare with an ejection. The flare onset phase 1Kondrashova NN, 1Pasechnik MN. Line-of-sight veloсity field in low atmosphere of an active region during a solar flare with an ejection. The flare onset phase. Russian. 2011 ;27(5):12-25.
On hydrodynamical mechanism of generation of global poloidal flow of the Sun 1Loginov AA, Sal'nikov NN, 1Cheremnykh OK, Zelyk YI, Maslova NV. On hydrodynamical mechanism of generation of global poloidal flow of the Sun. Russian. 2011 ;27(5):3-11.
Statistical characteristics of large sunspots in solar activity cycles 17-23 Babij VP, Efimenko VM, Lozitsky VG. Statistical characteristics of large sunspots in solar activity cycles 17-23. Russian. 2011 ;27(4):48-56.
Solar chromosphere in D₃ helium line from the spectra of the eclipse on 29 March 2006 Marchenko GP, 1Akimov LA, 1Belkina IL, Velikodsky YI. Solar chromosphere in D₃ helium line from the spectra of the eclipse on 29 March 2006. Russian. 2011 ;27(4):35-47.
Some properties of convective motions in the upper solar atmosphere. II 1Kostik RI. Some properties of convective motions in the upper solar atmosphere. II. Russian. 2011 ;27(4):24-34.
The influence of small scale magnetic fields on profiles of magnetically sensitive λ 525.02 nm and λ 1564.85 nm Fe I lines in the quiet solar photosphere 1Stodilka MI. The influence of small scale magnetic fields on profiles of magnetically sensitive λ 525.02 nm and λ 1564.85 nm Fe I lines in the quiet solar photosphere. 2011 ;27(4):3-23.
On 156-day quasi-periodicity of the solar indices Akimov LO, 1Belkina IL. On 156-day quasi-periodicity of the solar indices. Russian. 2011 ;27(3):40-53.