Using the data from the Interstellar Medium (ISM) we propose a physical model for the spectrum of the magnetic irregularities in the ISM. With this model we discuss the Galactic Cosmic Ray (GCR) spectrum, as well as the extragalactic Ultra High Energy Cosmic Rays (UHECRs), their chemical abundances and anisotropies. UHECRs may include a proton component from many radio galaxies integrated over vast distances, visible already below 3 EeV.
Using the data from the Interstellar Medium (ISM) we propose a physical model for the spectrum...
Department of Physics, Karlsruhe Institute for Technology KIT, Karlsruhe, Germany
Department of Physics & Astronomy, University of Alabama, Tuscaloosa, AL, USA
Department of Physics & Astronomy, University Bonn, Bonn, Germany
L. I. Caramete
Institute for Space Sciences, Bucharest, Romania
A. Meli
Department of Physics and Astronomy, University of Gent, Gent, Belgium
B. N. Nath
Raman Research Institute, Bangalore, India
E.-S. Seo
Department of Physics, University of Maryland, College Park, MD, USA
V. de Souza
University de São Paulo, Inst. de Física de São Carlos, São Carlos, Brazil
J. Becker Tjus
Department of Physics, University Bochum, Bochum, Germany
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Using the data from the Interstellar Medium (ISM) we propose a physical model for the spectrum of the magnetic irregularities in the ISM. With this model we discuss the Galactic Cosmic Ray (GCR) spectrum, as well as the extragalactic Ultra High Energy Cosmic Rays (UHECRs), their chemical abundances and anisotropies. UHECRs may include a proton component from many radio galaxies integrated over vast distances, visible already below 3 EeV.
Using the data from the Interstellar Medium (ISM) we propose a physical model for the spectrum...
