Results from AGASA experiment in the extremely high energy region

Details Results from AGASA experiment in the extremely high energy region Results from AGASA experiment in the extremely high energy region

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..433...76n&link_type=abstract

Workshop on observing giant cosmic ray air showers from >1020 eV particles from space. AIP Conference Proceedings, Volume 433, p

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Neutrino, Muon, Pion, And Other Elementary Particle Detectors, Cosmic Ray Detectors, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays

Scientific paper

Recent results on primary cosmic rays of energies above 1×1019 eV observed by the Akeno Giant Air Shower Array (AGASA) are summarized. It is likely that extremely high energy cosmic rays are from diffuse sources distributed isotropically in the universe. However, there are cosmic rays of energies in excess of the predicted cutoff energy and some fraction of cosmic rays beyond 4×1019 eV seem to come nearby sources composing double events within a limited space angle.

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