Computer Science
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7..260d&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 260-263 (SEE N85-35968 24-93)
Computer Science
Earth Atmosphere, Electrons, Gamma Rays, Hadrons, High Energy Interactions, Muons, Correlation, Distribution (Property)
Scientific paper
Distributions were calculated for the number of electrons Ne, number of muons with the energy above 5 GeV Nmu and the energy of hadron component Eh in electromagnetic showers, produced by primary gamma-quanta with energies theta approx. equals 30 deg and observed at the mountain level 700 g/square centimeters. The mean number of nuclear interactions of photos with the energy above 5 GeV is about 0.3 per each TeV of the primary energy and nuclear cascades take out in average about 2% of the total shower energy. The mean number of 5 GeV muons for the electromagnetic shower is (2 to 5)% from the number of muons in cosmic ray showers with the same number of electrons at the observation level. similar value for the total energy of hadron component is also (2 to 5)%. Nmu and Ne values as well as Eh and ne don't correlate at the fixed primary energy E sug gamma (o). Between Nmu and Eh there is a positive correlation at the given E sub gamma.
Danilova T. V.
Erlykin Anatoly D.
Mironov Aleksey V.
Tukish E. I.
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