Origin of hump in lateral distribution of Cherenkov photon density generated by gamma cosmic ray and study of its characteristics

Energetic secondary particles in gamma and hadron initiated showers can generate Cherenkov photons. Using CORSIKA code and simulation data, different characteristics of lateral distribution of Cherenkov photon density are studied. In particular, physical origin of these differences and also dependen...

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Main Authors: G Rastegarzadeh, M Najmi
Format: Article
Language:English
Published: Isfahan University of Technology 2010-12-01
Series:Iranian Journal of Physics Research
Subjects:
Online Access:http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-477&slc_lang=en&sid=1
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author G Rastegarzadeh
M Najmi
author_facet G Rastegarzadeh
M Najmi
author_sort G Rastegarzadeh
collection DOAJ
description Energetic secondary particles in gamma and hadron initiated showers can generate Cherenkov photons. Using CORSIKA code and simulation data, different characteristics of lateral distribution of Cherenkov photon density are studied. In particular, physical origin of these differences and also dependence of this distribution on primary energy and altitude of observation level are discussed. It is shown that the existence of a hump in lateral distribution of Cherenkov photon density in gamma initiated showers is a useful tool for separating gamma-hadron and rejecting hadron background in gamma ray astronomy.
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spelling doaj.art-8f7834221497491e8cf459bf6f8f3a3c2022-12-21T18:30:31ZengIsfahan University of TechnologyIranian Journal of Physics Research1682-69572010-12-01103169176Origin of hump in lateral distribution of Cherenkov photon density generated by gamma cosmic ray and study of its characteristicsG RastegarzadehM NajmiEnergetic secondary particles in gamma and hadron initiated showers can generate Cherenkov photons. Using CORSIKA code and simulation data, different characteristics of lateral distribution of Cherenkov photon density are studied. In particular, physical origin of these differences and also dependence of this distribution on primary energy and altitude of observation level are discussed. It is shown that the existence of a hump in lateral distribution of Cherenkov photon density in gamma initiated showers is a useful tool for separating gamma-hadron and rejecting hadron background in gamma ray astronomy.http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-477&slc_lang=en&sid=1CORSIKACherenkov photonsgamma ray astronomycosmic ray
spellingShingle G Rastegarzadeh
M Najmi
Origin of hump in lateral distribution of Cherenkov photon density generated by gamma cosmic ray and study of its characteristics
Iranian Journal of Physics Research
CORSIKA
Cherenkov photons
gamma ray astronomy
cosmic ray
title Origin of hump in lateral distribution of Cherenkov photon density generated by gamma cosmic ray and study of its characteristics
title_full Origin of hump in lateral distribution of Cherenkov photon density generated by gamma cosmic ray and study of its characteristics
title_fullStr Origin of hump in lateral distribution of Cherenkov photon density generated by gamma cosmic ray and study of its characteristics
title_full_unstemmed Origin of hump in lateral distribution of Cherenkov photon density generated by gamma cosmic ray and study of its characteristics
title_short Origin of hump in lateral distribution of Cherenkov photon density generated by gamma cosmic ray and study of its characteristics
title_sort origin of hump in lateral distribution of cherenkov photon density generated by gamma cosmic ray and study of its characteristics
topic CORSIKA
Cherenkov photons
gamma ray astronomy
cosmic ray
url http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-477&slc_lang=en&sid=1
work_keys_str_mv AT grastegarzadeh originofhumpinlateraldistributionofcherenkovphotondensitygeneratedbygammacosmicrayandstudyofitscharacteristics
AT mnajmi originofhumpinlateraldistributionofcherenkovphotondensitygeneratedbygammacosmicrayandstudyofitscharacteristics