Recent advances in measuring and interpreting cosmic rays from the spectral ankle to the highest energies are briefly reviewed. The prime question at the highest energies is about the origin of the flux suppression observed at E≃4{dot operator}1019eV. Is this the long-awaited GZK-effect or the exhaustion of sources? The key to answering this question will be provided by the largely unknown mass composition at the highest energies. The high level of isotropy observed even at the highest energies challenges models of a proton-dominated composition if extragalactic magnetic fields are on the order of a few nG or less. We shall discuss the experimental and theoretical progress in the field and the prospects for the next decade. © 2014 Académie ...
16 pages, 7 figuresThe significant attenuation of the cosmic ray flux above ~5 × 10^19 eV suggests t...
SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds...
SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds...
Received *****; accepted after revision +++++ Recent advances in measuring and interpreting cosmic r...
Recent advances in measuring and interpreting cosmic rays from the spectral ankle to the highest ene...
Observations of cosmic rays have been improved at all energies, both in terms of higher statistics a...
Abstract. Observations of cosmic rays have been improved at all energies, both in terms of higher st...
Abstract. After a century of observations, we still do not know the origin of cosmic rays. I will re...
International audienceThe origin of cosmic rays with energy E ≳ 1018 eV is a long-standing problem i...
16 pages, 7 figuresThe significant attenuation of the cosmic ray flux above ~5 × 10^19 eV suggests t...
16 pages, 7 figuresThe significant attenuation of the cosmic ray flux above ~5 × 10^19 eV suggests t...
16 pages, 7 figuresThe significant attenuation of the cosmic ray flux above ~5 × 10^19 eV suggests t...
16 pages, 7 figuresThe significant attenuation of the cosmic ray flux above ~5 × 10^19 eV suggests t...
SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds...
16 pages, 7 figuresThe significant attenuation of the cosmic ray flux above ~5 × 10^19 eV suggests t...
16 pages, 7 figuresThe significant attenuation of the cosmic ray flux above ~5 × 10^19 eV suggests t...
SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds...
SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds...
Received *****; accepted after revision +++++ Recent advances in measuring and interpreting cosmic r...
Recent advances in measuring and interpreting cosmic rays from the spectral ankle to the highest ene...
Observations of cosmic rays have been improved at all energies, both in terms of higher statistics a...
Abstract. Observations of cosmic rays have been improved at all energies, both in terms of higher st...
Abstract. After a century of observations, we still do not know the origin of cosmic rays. I will re...
International audienceThe origin of cosmic rays with energy E ≳ 1018 eV is a long-standing problem i...
16 pages, 7 figuresThe significant attenuation of the cosmic ray flux above ~5 × 10^19 eV suggests t...
16 pages, 7 figuresThe significant attenuation of the cosmic ray flux above ~5 × 10^19 eV suggests t...
16 pages, 7 figuresThe significant attenuation of the cosmic ray flux above ~5 × 10^19 eV suggests t...
16 pages, 7 figuresThe significant attenuation of the cosmic ray flux above ~5 × 10^19 eV suggests t...
SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds...
16 pages, 7 figuresThe significant attenuation of the cosmic ray flux above ~5 × 10^19 eV suggests t...
16 pages, 7 figuresThe significant attenuation of the cosmic ray flux above ~5 × 10^19 eV suggests t...
SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds...
SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds...