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Information × Registration Number 0308U008427, 0106U012581 , R & D reports Title The general and local characteristics of the Sun popup.stage_title Удосконалення програм для обробки спостережень Розрахунок теоретичних моделей. Head Stepanian Natalya, Registration Date 05-01-2009 Organization Scientific-research institute "Crimean astrophysical observatory" popup.description2 Two-component flare model was built by the use of spectral observations. The model determines the physical characteristics of the bright unresolved details. Magnetographic observations of the Sun with high spatial resolution testify to the presence of weak background field in the intervals between power tubes. The intensity of the background field is higher when the filling factor is bigger. It is shown that for the last 34 years the Sun pulsated with the period 159.966 min. This pulsation together with the well known oscillation P0=160.000 min generates the beating with the period 400(4) days. The evolution of the disbalance of the solar magnetic fields is determined by the coming out to the upper photosphere of the structures which rotate with the period, typical for zones of their formation. The drift of the structures to the poles and equator produces the creation of extended latitude zones with identical rotation and the appearance of the structures with different periods of rotation at the same latitude. Monitoring.5635 Product Description popup.authors popup.nrat_date 2020-04-02 Close