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Information × Registration Number 0208U000557, 0105U000546 , R & D reports Title The investigation of cosmic ray propagation in the magnetic fields of heliosphere popup.stage_title Head Shakhov Boris, Registration Date 01-02-2008 Organization Main Astronomical Observatory popup.description2 First the exact analytical solution of the Fokker-Planck kinetic equation in the second order of smallness on a pitch angle with allowance for of availability of focussing effect of cosmic rays (CR) by an interplanetary regular magnetic field against a background of its fluctuations is obtained. The technique of deriving of the information concerning spectra solar CR, generated near to the Sun, based on the exact analytical solutions of the transport equations is developed. The indexes of degree of spectra depending on distance up to the Sun for different functions of injection in a source are determined. The role of a multiplicity of neutrons for the registration galactic and solar CR by neutron monitors is investigated. The features of registration of the different astrophysical phenomena, which one are connected to energy of particles are found. On the basis of the diffusion theory is developed and is offered technique studying of an anisotropy of CR, accelerated on shockwaves, from rather closeto aheliosphere of supernova remnants. By the quantum theory field methods the parameters of a helical magnetohydrodynamic turbulence, which describe a particles acceleration in it, are obtained.56355635 Product Description popup.authors popup.nrat_date 2020-04-02 Close