Add to ORKGWe give a brief overview of the current experimental and theoretical status of cosmic rays above ~10**17 eV. We focus on the role of large scale magnetic fields and on multi-messenger aspects linking charged cosmic ray with secondary gamma-ray and neutrino fluxes
Observations of cosmic rays have been improved at all energies, both in terms of higher statistics a...
We briefly review the main channels of gamma ray and neutrino production due to the propagation of ul...
Abstract. Observations of cosmic rays have been improved at all energies, both in terms of higher st...
We give a brief (and highly incomplete) overview of the current experimental and theoretical status ...
7 pages, 2 figures, to appear in the proceedings of "The Dark Side of the Universe", Madrid, June 20...
7 pages, 2 figures, to appear in the proceedings of "The Dark Side of the Universe", Madrid, June 20...
7 pages, 2 figures, to appear in the proceedings of "The Dark Side of the Universe", Madrid, June 20...
7 pages, 2 figures, to appear in the proceedings of "The Dark Side of the Universe", Madrid, June 20...
7 pages, 2 figures, to appear in the proceedings of "The Dark Side of the Universe", Madrid, June 20...
7 pages, 2 figures, to appear in the proceedings of "The Dark Side of the Universe", Madrid, June 20...
Cosmic ray (CR) particles arrive at the top of the Earth's atmosphere at a rate of around 1000 per s...
The origin of cosmic rays is one of the major unresolved astrophysical questions. In particular, the...
A brief review of the energy spectrum of primary cosmic rays above $10^{10}$ eV and the measurement ...
We briefly review sources of cosmic rays, their composition and spectra as well as their propagation...
The most energetic particles ever detected exceed $10^{20}$ eV in energy. Their existence represents...
Observations of cosmic rays have been improved at all energies, both in terms of higher statistics a...
We briefly review the main channels of gamma ray and neutrino production due to the propagation of ul...
Abstract. Observations of cosmic rays have been improved at all energies, both in terms of higher st...
We give a brief (and highly incomplete) overview of the current experimental and theoretical status ...
7 pages, 2 figures, to appear in the proceedings of "The Dark Side of the Universe", Madrid, June 20...
7 pages, 2 figures, to appear in the proceedings of "The Dark Side of the Universe", Madrid, June 20...
7 pages, 2 figures, to appear in the proceedings of "The Dark Side of the Universe", Madrid, June 20...
7 pages, 2 figures, to appear in the proceedings of "The Dark Side of the Universe", Madrid, June 20...
7 pages, 2 figures, to appear in the proceedings of "The Dark Side of the Universe", Madrid, June 20...
7 pages, 2 figures, to appear in the proceedings of "The Dark Side of the Universe", Madrid, June 20...
Cosmic ray (CR) particles arrive at the top of the Earth's atmosphere at a rate of around 1000 per s...
The origin of cosmic rays is one of the major unresolved astrophysical questions. In particular, the...
A brief review of the energy spectrum of primary cosmic rays above $10^{10}$ eV and the measurement ...
We briefly review sources of cosmic rays, their composition and spectra as well as their propagation...
The most energetic particles ever detected exceed $10^{20}$ eV in energy. Their existence represents...
Observations of cosmic rays have been improved at all energies, both in terms of higher statistics a...
We briefly review the main channels of gamma ray and neutrino production due to the propagation of ul...
Abstract. Observations of cosmic rays have been improved at all energies, both in terms of higher st...