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astro-ph2005
Cosmic Ray Energy Measurement with EAS Cherenkov Light: Experiment QUEST and CORSIKA Simulation
E. E. Korosteleva, L. A. Kuzmichev, V. V. Prosin +1
A new method of a primary cosmic particle energy measurement with the extensive air shower (EAS) technique has been developed by exploiting: a) the joint analysis of the shower siz…
astro-ph2004
Primary Energy Measurement with EAS Cherenkov Light: Experiment QUEST and CORSIKA Simulation
E. Korosteleva, L. Kuzmichev, V. Prosin +2
A new primary mass independent method of energy measurement has been developed by exploiting: a) the joint analysis of the shower size, obtained by EAS-TOP, and of the EAS atmosphe…
astro-ph2003
The primary cosmic ray composition between 10**15 and 10**16 eV from Extensive Air Showers electromagnetic and TeV muon data
TOP Collaboration, MACRO Collaboration
The cosmic ray primary composition in the energy range between 10**15 and 10**16 eV, i.e., around the "knee" of the primary spectrum, has been studied through the combined measurem…