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- W1483179985 abstract "We consider the propagation and source distribution of cosmic rays. The principal requirement for the various models we consider is that they should be capable of holding particles in dense regions of the galactic disk for periods of time sufficient to produce the observed fragmentation products of cosmic rays. This can be achieved by both simple and compound diffusion provided that suitable mean free paths and boundary conditions are chosen. The bulk of the anisotropy is caused by the discrete nature of the cosmic ray sources. However, models which reproduce the fragmentation products will in general yield anisotropies consistent with available upper limits." @default.
- W1483179985 created "2016-06-24" @default.
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- W1483179985 date "1971-01-01" @default.
- W1483179985 modified "2023-09-27" @default.
- W1483179985 title "The effects of propagation and source distribution on cosmic ray composition and anisotropy." @default.
- W1483179985 hasPublicationYear "1971" @default.
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