Energy spectra of leading secondary particles in hadron-nuclei interactions

Details Energy spectra of leading secondary particles in hadron-nuclei interactions Energy spectra of leading secondary particles in hadron-nuclei interactions

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976izssr..40..947a&link_type=abstract

(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Samarkand, Uzbek SSR, Oct. 29-31, 1975.) Akademiia Nauk SSSR, Izvest

Other

Cosmic Ray Showers, Energy Spectra, Hadrons, Ionization Chambers, Nuclear Interactions, Absorbers (Materials), Heavy Nuclei, Iron, Least Squares Method, Monte Carlo Method

Scientific paper

One calorimeter employed at the Aragats mountain station (3220 m above sea level) was composed of 16 rows of ionization chambers of rectangular cross section with 7.5-cm-thick iron between the chambers. The total absorber thickness was 1040 g/sq cm. The other calorimeter was composed of 10 rows of ionization chambers of circular cross section separated by 10-cm-thick iron layers with a total absorber thickness of 840 g/sq cm. The energy spectra of the leading secondaries are analyzed on the basis of data on the interaction of cosmic hadrons with the iron nuclei.

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