Narrow-angle cosmic-ray anisotropies

Astronomy and Astrophysics – Astronomy

Scientific paper

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Anisotropy, Cosmic Rays, Diurnal Variations, Galactic Radiation, Interstellar Magnetic Fields, Particle Flux Density, Astronomical Models, Energy Distribution, Particle Diffusion, Particle Energy, Primary Cosmic Rays, Solar Activity Effects

Scientific paper

An alternate interpretation is presented for the diurnal cosmic ray anisotropy measurements made with underground muons in London. From the widely accepted models of cosmic ray diffusion in the Galaxy, a diurnal anisotropy (24 h wave) would be expected. But from a model predicting the occurrence of an excess within some small region of the celestial sphere, it is suggested that the direction of this excess would depend on the orientation (in space and time) of the source relative to galactic magnetic field lines which connect the source with the solar system.

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