Study of the longitudinal development of individual EAS inferred from the Cherenkov light pulse shape: method and results

1986 ◽  
Vol 248 (1) ◽  
pp. 227-233 ◽  
Author(s):  
Yu.A. Fomin ◽  
G.B. Khristiansen
Keyword(s):  
Light Pulse ◽  
Pulse Shape ◽  
Cherenkov Light ◽  
Longitudinal Development

scholarly journals PRIMARY ENERGY SPECTRUM AND MASS COMPOSITION DETERMINED WITH THE TUNKA EAS CHERENKOV ARRAY

2005 ◽  
Vol 20 (29) ◽  
pp. 6799-6801 ◽  
Author(s):  
D. V. CHERNOV ◽  
E. E. KOROSTELEVA ◽  
L. A. KUZMICHEV ◽  
V. V. PROSIN ◽  
I. V. YASHIN ◽  
...  
Keyword(s):  
Monte Carlo ◽  
Distribution Function ◽  
Energy Spectrum ◽  
Monte Carlo Simulations ◽  
Light Pulse ◽  
Primary Energy ◽  
Cherenkov Light ◽  
Mass Composition ◽  
Knee Region ◽  
The Mean

New results of 300 hours of operation of the TUNKA array are presented. An improved parametrization of the Cherenkov light lateral distribution function (LDF), based on CORSIKA Monte Carlo simulations and the experiment QUEST, has been used for the reconstruction of EAS parameters. The corrected energy spectrum in the knee region is obtained. The mean depth of the EAS maximum has been derived both from the analysis of LDF steepness and the FWHM of Cherenkov light pulse. The mean mass composition around the knee is estimated.

Light Pulse Shape Dependence on $\gamma$-Ray Energy in CsI(Tl)

2008 ◽  
Vol 55 (3) ◽  
pp. 1246-1250 ◽  
Author(s):  
Agnieszka Syntfeld-Kazuch ◽  
Marek Moszynski ◽  
Lukasz Swiderski ◽  
Wlodzimierz Klamra ◽  
Antoni Nassalski
Keyword(s):  
Light Pulse ◽  
Pulse Shape ◽  
Gamma Ray ◽  
Shape Dependence

Calibrating the light pulse shape of a hydrogen flashlamp using synchrotron radiation as a standard of excitation

1979 ◽  
Vol 18 (9) ◽  
pp. 1355 ◽  
Author(s):  
J. C. Andre ◽  
R. Lopez-Delgado ◽  
R. L. Lyke ◽  
W. R. Ware
Keyword(s):  
Synchrotron Radiation ◽  
Light Pulse ◽  
Pulse Shape

Solar Flare Energetic Neutral Emission Measurements in the Project Coronas-I

1994 ◽  
Vol 144 ◽  
pp. 635-639
Author(s):  
J. Baláž ◽  
A. V. Dmitriev ◽  
M. A. Kovalevskaya ◽  
K. Kudela ◽  
S. N. Kuznetsov ◽  
...  
Keyword(s):  
Solar Flare ◽  
Energy Range ◽  
Gamma Rays ◽  
Pulse Shape ◽  
Gamma Ray ◽  
Pulse Shape Discrimination ◽  
Shape Discrimination ◽  
Solar Neutron ◽  
Low Altitude

AbstractThe experiment SONG (SOlar Neutron and Gamma rays) for the low altitude satellite CORONAS-I is described. The instrument is capable to provide gamma-ray line and continuum detection in the energy range 0.1 – 100 MeV as well as detection of neutrons with energies above 30 MeV. As a by-product, the electrons in the range 11 – 108 MeV will be measured too. The pulse shape discrimination technique (PSD) is used.

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