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Aleksandrov, L.; Brankova, M.; Kirov, I.; Mavrodiev, S.Cht.; Mishev, A.; Stamenov, J.; Ushev, S.
Bogolyubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna (Russian Federation); Institute for Nuclear Research and Nuclear Energy, Sofia (Bulgaria)1998
Bogolyubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna (Russian Federation); Institute for Nuclear Research and Nuclear Energy, Sofia (Bulgaria)1998
AbstractAbstract
[en] A method for analysis of extensive air showers initiated by primary gamma quanta of primary protons and nuclei in the atmosphere is presented. The method is based on measuring of Cherenkov light distribution in showers. A new approximation of the lateral and radial distributions is obtained on the basis of a nonlinear overdetermined inverse problem solution. The concrete mathematical model is created by analysis of recent measurements carried out by the Cherenkov wide angle timing telescope HOTOVO. The model is tested on simulated data obtained with the code CORSIKA. The method is applied to different sets of detectors of CELESTE array. A new detector array for optimal estimation of Cherenkov flux parameters is proposed
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Source
1998; 10 p; 9 refs., 8 figs., 5 tabs.
Record Type
Report
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Country of publication
ASTRONOMY, BARYONS, BOSONS, CATIONS, CHARGED PARTICLES, COSMIC RADIATION, COSMIC SHOWERS, DISTRIBUTION, ELEMENTARY PARTICLES, ENERGY RANGE, FERMIONS, GEV RANGE, HADRONS, HYDROGEN IONS, HYDROGEN IONS 1 PLUS, IONIZING RADIATIONS, IONS, MASSLESS PARTICLES, MEASURING INSTRUMENTS, NUCLEI, NUCLEONS, PHOTONS, PRIMARY COSMIC RADIATION, PROTONS, RADIATIONS, SECONDARY COSMIC RADIATION, SHOWERS, SPECTRA, SPECTROMETERS, TEV RANGE
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