Calculation of magnetic fields in the solar corona during the total solar eclipse on 1 August 2008 in the potential approach

¹Pishkalo MI. Calculation of magnetic fields in the solar corona during the total solar eclipse on 1 August 2008 in the potential approach. Russian. 2010 ;26(3):15-33.

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.

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