Determination of the solar radius from total solar eclipse photometric observations

Danylevskyi VO. Determination of the solar radius from total solar eclipse photometric observations. 2004 ;20(2):176-188.

Dynamics of magneto-hydrodynamical oscillations from observations of the solar active region NOAA 0119 over a range of wavelengths from 2.0 to 107 cm

Budzinovskaia IA, Tsvetkov LI, ¹Yurovsky YF. Dynamics of magneto-hydrodynamical oscillations from observations of the solar active region NOAA 0119 over a range of wavelengths from 2.0 to 107 cm. 2004 ;20(2):165-175.

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.

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