Lateral distribution of Cherenkov light in extensive air showers at high mountain altitude produced by different primary particles in wide energy range

Simple item page
dc.creatorMishev, A.
dc.creatorStamenov, J.
dc.date2005-12-16
dc.date.accessioned2026-07-07T06:49:09Z
dc.date.available2026-07-07T06:49:09Z
dc.descriptionThe general aim of this work is to obtain the lateral distribution of atmospheric Cherenkov light in extensive air showers produced by different primary particles precisely by. protons, Helium, Iron, Oxygen, Carbon, Nitrogen, Calcium, Silicon and gamma quanta in wide energy range at high mountain observation level of Chacaltaya cosmic ray station. The simulations are divided generally in two energy ranges 10GeV-10 TeV and 10 TeV-10 PeV. One large detector has been used for simulations, the aim being to reduce the statistical fluctuations of the obtained characteristics. The shape of the obtained lateral distributions of Cherenkov light in extensive air showers is discussed and the scientific potential for solution of different problems as well.
dc.description19 pages, 21 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0512432
dc.identifierhttp://arxiv.org/abs/astro-ph/0512432
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/104230
dc.subjectAstrophysics
dc.titleLateral distribution of Cherenkov light in extensive air showers at high mountain altitude produced by different primary particles in wide energy range
dc.typetext

Files

Collections

arXiv