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Calculations of the cosmic ray modulation in interplanetary space taking into account the possible dependence of the transport travel for the scattering of the particles and of the velocity of the solar winds on the angles they make with the helioequator plane: The case of isotropic diffusionThe modulation of galactic cosmic rays is studied by the magnetic heterogeneities stream on the assumption that the diffusion coefficient is reduced whereas the solar wind velocity is increased with the growth of the angle between the sun's rotation axis and the direction of solar plasma motion. The stationary plane problem of isotropic diffusion is solved as it applies to two cases: (1) with due account of particle retardation by the antiphermium mechanism; and (2) without an account of the above mechanism. This problem is solved by the grid method in the polar coordinate system. The results of the calculations are followed by a discussion of the method of solution and of the errors.
Document ID
19750008395
Acquisition Source
Legacy CDMS
Document Type
Book
Authors
Dorman, L. I.
(Kanner (Leo) Associates Redwood City, CA, United States)
Kobilinski, Z.
(Kanner (Leo) Associates Redwood City, CA, United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1975
Publication Information
Publication: Cosmic Rays (
Subject Category
Space Radiation
Accession Number
75N16467
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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