Physics
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8..210i&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 8 p 210-213 (SEE N85-36066 24-93)
Physics
2
Cosmic Rays, Flux Density, High Energy Interactions, Muons, Angular Distribution, Data Reduction, Emulsions, Energy Spectra, Gamma Rays
Scientific paper
The overall data from the investigation of the cosmic ray muon flux in the range of zenith angles (0-90) deg within the energy range (3.5 to 5.0) TeV is presented. The exposure of large X-ray emulsion chambers underground was 1200 tons. year. The data were processe using the method which was applied in the experiment Pamir and differred from the earlier applied one. The obtained value of a slope power index of the differential energy spectrum of the global muon flux is =3.7 that corresponds to the slope of the pion generation differential spectrum, gammaPI = 2.75 + or - .04. The analysis of the muon zenith-angular distribution showed that the contribution of rapid generation muons in the total muon flux agree the best with the value .2% and less with .7% at a 90% reliability level.
Ilyina N. P.
Ivanenko I. P.
Ivanova Marina A.
Kuz'michev L. A.
Mandritskaya K. V.
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