Mass composition of cosmic rays in the range 2×1017–3×1018 eV measured with the Haverah Park array
- 1 August 2002
- journal article
- Published by Elsevier in Astroparticle Physics
- Vol. 19 (1) , 61-75
- https://doi.org/10.1016/s0927-6505(02)00189-5
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This publication has 11 references indexed in Scilit:
- Measurement of the Cosmic‐Ray Energy Spectrum and Composition from 1017to 1018.3eV Using a Hybrid TechniqueThe Astrophysical Journal, 2001
- Comparison of AGASA data with CORSIKA simulationAstroparticle Physics, 2000
- Charmless decays of theB-meson in perturbative QCDJournal of Physics G: Nuclear and Particle Physics, 1999
- The lateral distribution of extensive air showers produced by cosmic rays above 1019 eV as measured by water-Čerenkov detectorsAstroparticle Physics, 1997
- Quark-gluon-string model and EAS simulation problems at ultra-high energiesNuclear Physics B - Proceedings Supplements, 1997
- Cosmic-ray composition aroundeVPhysical Review D, 1993
- The cosmic ray energy spectrum above 4*1017eV as measured by the Haverah Park arrayJournal of Physics G: Nuclear and Particle Physics, 1991
- A coarse-grain search for anisotropy in the arrival directions of cosmic rays above 10 to the 17th eVThe Astrophysical Journal, 1990
- Measurement of the elongation rate of extensive air showers produced by primary cosmic rays of energy above 2×1017eVJournal of Physics G: Nuclear Physics, 1981
- Fluctuation studies of large air showers: the composition of primary cosmic ray particles of energy Ep∼1018eVJournal of Physics A: Mathematical, Nuclear and General, 1974