Prediction of maximum of Solar cycle 25: total power at the cycle beginning and in the previous cycle as precursor

¹Pishkalo MI, Vasiljeva IE. Prediction of maximum of Solar cycle 25: total power at the cycle beginning and in the previous cycle as precursor. Ukrainian. 2023 ;39(4):68-89.

Fe I line pairs of different magnetic sensitivity

¹Vasilyeva IE, ¹Shchukina NG. Fe I line pairs of different magnetic sensitivity. 2009 ;25(6):482-489.

The simulation of the photosphere and chromosphere of two big solar flares (on 28 October 2003 and 1 September 1990

¹Baranovsky EA, Lozitsky VG, Tarashchuk VP). The simulation of the photosphere and chromosphere of two big solar flares (on 28 October 2003 and 1 September 1990. 2009 ;25(5):373-384.

Solar corona during the total solar eclipse on August 1, 2008

¹Pishkalo MI, Baransky AR. Solar corona during the total solar eclipse on August 1, 2008. 2009 ;25(6):474-481.

Photometric flattening index of the Solar corona in the Solar cycle

¹Pishkalo MI. Photometric flattening index of the Solar corona in the Solar cycle. 2023 ;39(3):67-78.

Early forecast of maximum of 25th cycle of Solar activity

Lozitsky VG, Efimenko VM. Early forecast of maximum of 25th cycle of Solar activity. 2023 ;39(1):65-71.

Torsional oscillations of umbra and penumbra of sunspots

¹Gopasyuk OS. Torsional oscillations of umbra and penumbra of sunspots. Russian. 2010 ;26(5):41-49.

Properties of convective motions in the upper solar atmosphere. I

¹Kostik RI. Properties of convective motions in the upper solar atmosphere. I. Russian. 2010 ;26(5):26-40.

Fine structure of the velocity field in an importance 2B/M2.3 flare

Babin AN, Koval AN. Fine structure of the velocity field in an importance 2B/M2.3 flare. Russian. 2010 ;26(3):50-57.

The field of horizontal convective velocities from observations on the solar limb

¹Baran OA, ¹Stodilka MI. The field of horizontal convective velocities from observations on the solar limb. 2010 ;26(3):34-49.

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