The mass composition of cosmic rays near 1018 eV as deduced from measurements made at Volcano Ranch
Open Access
- 30 September 2004
- journal article
- Published by Elsevier in Astroparticle Physics
- Vol. 21 (6) , 597-607
- https://doi.org/10.1016/j.astropartphys.2004.04.009
Abstract
No abstract availableKeywords
All Related Versions
This publication has 16 references indexed in Scilit:
- Geant4—a simulation toolkitNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2003
- Mass composition of cosmic rays in the range 2×1017–3×1018 eV measured with the Haverah Park arrayAstroparticle Physics, 2002
- 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
- Evidence for Changing of Cosmic Ray Composition betweenandeV from Multicomponent MeasurementsPhysical Review Letters, 2000
- A comparison of cosmic ray composition measurements at the highest energiesAstroparticle Physics, 1998
- Quark-gluon-string model and EAS simulation problems at ultra-high energiesNuclear Physics B - Proceedings Supplements, 1997
- Muons (>or=1 GeV) in large extensive air showers of energies between 1016.5eV and 1019.5eV observed at AkenoJournal of Physics G: Nuclear and Particle Physics, 1995
- The cosmic ray energy spectrum above 3 × 1018 eV measured by the Akeno Giant Air Shower ArrayAstroparticle Physics, 1995
- Evidence for correlated changes in the spectrum and composition of cosmic rays at extremely high energiesPhysical Review Letters, 1993