The cosmic ray primary composition between 1015 and 1016 eV from Extensive Air Showers electromagnetic and TeV muon data
- 31 March 2004
- journal article
- Published by Elsevier in Astroparticle Physics
- Vol. 20 (6) , 641-652
- https://doi.org/10.1016/j.astropartphys.2003.10.004
Abstract
No abstract availableKeywords
All Related Versions
This publication has 20 references indexed in Scilit:
- Muon density measurements with the KASCADE central detectorAstroparticle Physics, 2001
- The EAS size spectrum and the cosmic ray energy spectrum in the region 1015–1016 eVAstroparticle Physics, 1999
- Cosmic ray studies around the “knee” of the primary spectrum from EAS-TOPNuclear Physics B - Proceedings Supplements, 1998
- A three-dimensional code for muon propagation through the rock: MUSICAstroparticle Physics, 1997
- A single source of cosmic rays in the range - eVJournal of Physics G: Nuclear and Particle Physics, 1997
- Study of the primary cosmic ray composition around the knee of the energy spectrumPhysics Letters B, 1994
- UHE cosmic ray event reconstruction by the electromagnetic detector of EAS-TOPNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 1993
- First supermodule of the MACRO detector at Gran SassoNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 1993
- Measurement of the decoherence function with the MACRO detector at Gran SassoPhysical Review D, 1992
- Simultaneous observation of extensive air showers and deep-underground muons at the Gran Sasso LaboratoryPhysical Review D, 1990