Reconstruction of source and cosmic magnetic field characteristics from clusters of ultra-high energy cosmic rays
- 30 June 1998
- journal article
- Published by Elsevier in Astroparticle Physics
- Vol. 9 (1) , 65-78
- https://doi.org/10.1016/s0927-6505(98)00006-1
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- Possible Clustering of the Most Energetic Cosmic Rays within a Limited Space Angle Observed by the Akeno Giant Air Shower ArrayPhysical Review Letters, 1996
- Arrival Directions of the Most Energetic Cosmic RaysPhysical Review Letters, 1995
- In search of a source for the 320 EeV Fly's Eye cosmic rayThe Astrophysical Journal, 1995
- Detection of a cosmic ray with measured energy well beyond the expected spectral cutoff due to cosmic microwave radiationThe Astrophysical Journal, 1995
- The cosmic ray energy spectrum above 3 × 1018 eV measured by the Akeno Giant Air Shower ArrayAstroparticle Physics, 1995
- Observation of a Very Energetic Cosmic Ray Well Beyond the Predicted 2.7 K Cutoff in the Primary Energy SpectrumPhysical Review Letters, 1994
- The cosmic-ray energy spectrum observed by the Fly's EyeThe Astrophysical Journal, 1994
- Evidence for correlated changes in the spectrum and composition of cosmic rays at extremely high energiesPhysical Review Letters, 1993
- The cosmic ray energy spectrum above 4*1017eV as measured by the Haverah Park arrayJournal of Physics G: Nuclear and Particle Physics, 1991
- End to the Cosmic-Ray Spectrum?Physical Review Letters, 1966