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Information × Registration Number 0218U002479, 0112U007812 , R & D reports Title The interaction of cosmic rays with turbulent magnetic fields of the heliosphere and interstellar medium popup.stage_title Head Shakhov Boris, Registration Date 21-03-2018 Organization Main Astronomical Observatory popup.description2 Based on the study of the statistical acceleration of cosmic rays in a turbulent medium, it is shown that the equilibrium spatial-energy distribution of accelerated particles is determined by the efficiency of their acceleration and the characteristics of the diffusion propagation of cosmic rays in the acceleration region and beyond. Proceeding from the solutions of the transport equation for cosmic rays, the space-time distribution of solar cosmic rays and the dynamics of their energy spectrum were investigated. The distribution of cosmic rays of ultra high energies in intergalactic magnetic fields and the evolution of energy spectra of charged particles of ultrahigh energies accelerated by a local source have been investigated. Based on the data of the global network of neutron monitors, the intensity of galactic cosmic rays in the Forbush effects periods was investigated. The process of the appearance of plasma instabilities and the generation of turbulence in the region of the Earth's magnetosphere have been investigated. The role of turbulence in the formation of the sporadic plasma layer of the lower ionosphere have been investigated. Product Description popup.authors Кизьюров Ю.В. Клюєва А.І. Колесник Ю.Л. Маловічко П.П. Федоров Ю.І Шахов Б. О. popup.nrat_date 2020-04-02 Close