On the rotation of solar large-scale magnetic fields of the opposite polarity 1Leiko UM. On the rotation of solar large-scale magnetic fields of the opposite polarity. 2004 ;20(1):34-42.
The electric field and charge in the solar corona 1Yefimenko VM, 2Tokii VV, 2Tokii NV. The electric field and charge in the solar corona. 2004 ;20(1):27-33.
2-D MHD model of solar magnetogranulation. Dynamics of magnetic elements 1Sheminova VA. 2-D MHD model of solar magnetogranulation. Dynamics of magnetic elements. 2004 ;20(1):3-26.
The height of the polar chromosphere in 2012—2023 according to observations on the Ernest Gurtovenko telescope Osipov SM, 1Pishkalo MI. The height of the polar chromosphere in 2012—2023 according to observations on the Ernest Gurtovenko telescope. 2024 ;40(6):73-85.
Comparison of direct magnetic field measurements in a sunspot by ten spectral lines of Fe I, Fe II, Ti I and Ti II Lozitska NI, Yakovkin II, Lozitsky VG, Hromov MA. Comparison of direct magnetic field measurements in a sunspot by ten spectral lines of Fe I, Fe II, Ti I and Ti II. 2024 ;40(6):59-72.
Sensitivity of the Fe IX 17.1 nm line profile to slow magneto-acoustic waves propagating in a solar coronal loop 1Mamedov SG, Aliyeva ZF, Samedov ZA. Sensitivity of the Fe IX 17.1 nm line profile to slow magneto-acoustic waves propagating in a solar coronal loop. 2024 ;40(6):45-58.
Spectral study of activ region site with Ellerman bomb and Hα-ejections. Chromosphere. Arch filament system 1Pasechnik MN. Spectral study of activ region site with Ellerman bomb and Hα-ejections. Chromosphere. Arch filament system. 2024 ;40(5):40-72.
A statistical study of the CME properties based on angular width during the solar cycle 24 1Dharmashaktu H, 2Lohani NK. A statistical study of the CME properties based on angular width during the solar cycle 24. 2024 ;40(4):3-21.
On long-term variations of the total irradiance and on probable changes of temperature in the Sun's core 1Abdussamatov HI. On long-term variations of the total irradiance and on probable changes of temperature in the Sun's core. 2005 ;21(6):471-477.
Diagnostics of the solar atmosphere by inverse methods: hydrogen absorption lines 1Stodilka MI. Diagnostics of the solar atmosphere by inverse methods: hydrogen absorption lines. 2005 ;21(6):461-470.