Autor: |
Al-Rubaiee, A. A., Gress, O. A., Lokhtin, K. S., Parfenov, Yu. V., Sinegovskii, S. I. |
Předmět: |
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Zdroj: |
Russian Physics Journal; Oct2005, Vol. 48 Issue 10, p1004-1011, 8p, 1 Chart, 6 Graphs |
Abstrakt: |
Spatial distribution of Čerenkov radiation of extensive air shower particles with energies 1013–1016 eV is simulated by the CORSIKA code for conditions and configuration of the Tunka-25 facility. Based on the calculated results, sets of approximating functions are constructed for different primary particles and zenith angles. A comparison of the calculated spatial distribution functions of Čerenkov light with the functions measured on the Tunka-25 facility demonstrates the feasibility of identification of the particle initiating the shower and determination of its energy in the vicinity of the bend point of the cosmic ray spectrum. [ABSTRACT FROM AUTHOR] |
Databáze: |
Complementary Index |
Externí odkaz: |
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