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Information × Registration Number 0217U003567, 0114U007387 , R & D reports Title The wave processes caused by instabilities in magnetized turbulent plasma and its influence on generation and distribution of high-energy charged particles popup.stage_title Head Kryshtal O.N., Registration Date 22-05-2017 Organization Main Astronomical Observatory popup.description2 It was found and carefully studied the new mechanism of occurrence of low-frequency turbulence near shock waves - compensated current instability. The peculiarities of the development of hose instability in the pre-shock region of the earth's bow shock wave are studied, with propagation of reflected, intermediate and diffusion beams. New results are obtained on the role of turbulence in the formation of the sporadic Es plasma layer of the Earth's ionosphere. The effect of high-power radio waves on the properties of the lower ionosphere is investigated. New results are obtained on the backscattering of radio waves on the electron concentration inhomogeneities of lower ionosphere plasmas. A new mechanism of electromagnetic radiation that can be responsible for the occurrence of solar radio bursts of I-th type is proposed. The generation of the second harmonic of quasi-Bernstein modes in the deco-hectogous range of the magnetic field amplitudes in arched structures in the pre-flare atmosphere of the active region on the Sun is considered. New important results have been obtained that make it possible to improve the outbreak prediction in the chromosphere of the active region on the Sun. The oscillations of a cylinder with a helical magnetic field are investigated. The results of the work can be used to interpret the dynamics of magnetic tubes in the Earth's magnetosphere, as well as in the atmosphere of the Sun. Product Description popup.authors Войцеховська Анна Дмитрівна Герасименко Світлана Володимирівна Кизьюров Ю.В. Кришталь Олександр Нектарович Любчик О.К. Маловічко П.П. popup.nrat_date 2020-04-02 Close