Abstract

The paper proposes a model in which the cosmic ray spectrum is formed by propagation processes in magnetic and photon fields of Galaxy, for energy range from JACEE to Fly’s Eye experiments. The turbulence effect of Galactic magnetic field on the propagation of cosmic ray nuclei has been investigated. We have found that the way of propagation of the protons (and nuclei respectively) is changed at the same energies where JACEE and Fly’s Eye experiments observe alteration in the spectrum of protons. The diffusion equations for the nuclei in field of soft photons and turbulent magnetic field have been solved. We argue that the anisotropy of secondary protons should follow the heavy nuclei one. A good agreement with the whole features in total cosmic ray energy spectrum was obtained for parameters widely accepted for the cosmic environment.

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.