On the possibility of the development of longitudinal wave instabilities on the background of the small-scale Bernstein turbulence in preflare chromosphere of a solar active region

¹Kryshtal AN, ¹Voitsekhovska AD, ¹Gerasimenko SV, ²Sidorenko MV. On the possibility of the development of longitudinal wave instabilities on the background of the small-scale Bernstein turbulence in preflare chromosphere of a solar active region. Russian. 2014 ;30(5):39-55.

Peculiarities of solar photospheric convection at granular, mesogranular and supergranular scales

¹Baran OA, ¹Stodilka MI. Peculiarities of solar photospheric convection at granular, mesogranular and supergranular scales. Ukrainian. 2014 ;30(4):23-37.

Plasma motions in the solar loop of the emerging magnetic flux

¹Pasechnik MN. Plasma motions in the solar loop of the emerging magnetic flux. Russian. 2014 ;30(4):3-22.

On one type of three-wave interaction of low-frequency waves in magnetoactive plasma of the solar atmosphere

¹Kryshtal AN, ¹Gerasimenko SV, ¹Voitsekhovska AD, ²Cheremnykh OK. On one type of three-wave interaction of low-frequency waves in magnetoactive plasma of the solar atmosphere. Russian. 2014 ;30(3):58-70.

Two-component photospheric models of a solar flare of 2N/M2 class

¹Andriiets OS, ²Kondrashova NN, ¹Kurochka EV. Two-component photospheric models of a solar flare of 2N/M2 class. Russian. 2014 ;30(2):58-69.

The influence of magnetic field on the propagation of 5-min oscillations in the solar atmosphere: the phase shifts

¹Kostyk RI, ¹Shchukina NG, ²Kobanov NI, ²Pulyaev VA. The influence of magnetic field on the propagation of 5-min oscillations in the solar atmosphere: the phase shifts. Russian. 2014 ;30(1):61-69.

Pre-flare changes of the solar photosphere using THEMIS observations data

¹Andriiets OS, ²Kondrashova NN. Pre-flare changes of the solar photosphere using THEMIS observations data. Russian. 2014 ;30(1):50-60.

Some problems of asymmetry of coronal spectral lines

¹Mamedov SG, ²Kuli-Zade DM, ¹Ismailli RF. Some problems of asymmetry of coronal spectral lines. Russian. 2015 ;31(5):49-60.

Power of the energy of the 11-year solar cycle and its dependence on the duration of the solar cycle

¹Abdussamatov HI. Power of the energy of the 11-year solar cycle and its dependence on the duration of the solar cycle. Russian. 2015 ;31(4):54-60.

What mechanisms allow the 5-minute oscillations in the active regions of the solar surface to penetrate from the photosphere into the chromosphere?

¹Kostyk RI. What mechanisms allow the 5-minute oscillations in the active regions of the solar surface to penetrate from the photosphere into the chromosphere?. Russian. 2015 ;31(4):45-53.

Pages