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Information × Registration Number 0213U003543, 0108U000208 , R & D reports Title Cosmic ray accelaration and propagation in the Solar wind popup.stage_title Head Shakhov Boris, Registration Date 07-02-2013 Organization Main Astronomical Observatory popup.description2 Received the intensity distribution function, anisotropy, and cosmic ray energy spectra during their propagation in the solar wind, which correspond to the latest models of the heliosphere. Found that regardless of the ratio of diffusion coefficients in a medium consisting of internal and external area of the heliosphere and heliosferic mantle at termination shock and heliopause there are more high energy particles than in the interstellar medium, whereas on the contrary there are less low-energy particles. The estimation of the duration of injection and transport path of solar cosmic rays in the interplanetary medium for several solar proton events was evaluated, which are characterized by large anisotropy that persists for a long period of time. Product Description popup.authors Іванов М.О. Колесник Ю.Л. Федоров Ю.І Шахов Б. О. popup.nrat_date 2020-04-02 Close