Add to ORKGThe lateral distribution of atmospheric Cerenkov photons emitted by gamma ray showers of energy 100 GeV is calculated. The lateral distribution shows a characteristic hump at a distance of approx. 135 meter from the core. The hump is shown to be due to electrons of threshold energy 1 GeV, above which the mean scattering angle becomes smaller than the Cerenkov angle
The discrimination between air showers initiated by #gamma# rays and by hadrons is one of the fundam...
This work summarizes the results presented at 29th International Cosmic Ray Conference in Pune India...
The facility designed for the study of angular resolution of light in the extensive air showers EAS ...
Investigations of the cosmic ray flux around the " knee " in the all - particle energy spectrum can ...
Characteristics of the direct and scattered components of electron-photon shower optical radiation f...
Energetic secondary particles in gamma and hadron initiated showers can generate Cherenkov photons. ...
This thesis reports measurements made on the longitudinal cascade of high energy cosmic ray showers ...
Abstract. The EAS Cherenkov radiation in the showers with energies 1015 ÷ 1017 eV has been measured....
It is shown that it should be possible to distinguish very effectively between background hadronic s...
An experiment designed to measure Cerenkov radiation from cosmic ray extensive air showers was deplo...
Atmospheric Cerenkov telescopes are used to detect electromagnetic showers from primary gamma rays o...
A high energy event of a bundle of electrons, gamma rays and hadronic gamma rays in an air shower co...
Lateral distribution of charged particles which allow for the finiteness of energy gamma-quanta, the...
The details of Cerenkov light produced by a gamma ray or a cosmic ray incident at the top of the atm...
A new knee-like approximation of the lateral distribution function (LDF) of EAS Cherenkov light in t...
The discrimination between air showers initiated by #gamma# rays and by hadrons is one of the fundam...
This work summarizes the results presented at 29th International Cosmic Ray Conference in Pune India...
The facility designed for the study of angular resolution of light in the extensive air showers EAS ...
Investigations of the cosmic ray flux around the " knee " in the all - particle energy spectrum can ...
Characteristics of the direct and scattered components of electron-photon shower optical radiation f...
Energetic secondary particles in gamma and hadron initiated showers can generate Cherenkov photons. ...
This thesis reports measurements made on the longitudinal cascade of high energy cosmic ray showers ...
Abstract. The EAS Cherenkov radiation in the showers with energies 1015 ÷ 1017 eV has been measured....
It is shown that it should be possible to distinguish very effectively between background hadronic s...
An experiment designed to measure Cerenkov radiation from cosmic ray extensive air showers was deplo...
Atmospheric Cerenkov telescopes are used to detect electromagnetic showers from primary gamma rays o...
A high energy event of a bundle of electrons, gamma rays and hadronic gamma rays in an air shower co...
Lateral distribution of charged particles which allow for the finiteness of energy gamma-quanta, the...
The details of Cerenkov light produced by a gamma ray or a cosmic ray incident at the top of the atm...
A new knee-like approximation of the lateral distribution function (LDF) of EAS Cherenkov light in t...
The discrimination between air showers initiated by #gamma# rays and by hadrons is one of the fundam...
This work summarizes the results presented at 29th International Cosmic Ray Conference in Pune India...
The facility designed for the study of angular resolution of light in the extensive air showers EAS ...