Other
Scientific paper
Jun 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993eme..work....1b&link_type=abstract
In Tokyo Univ., Contributions to the 23rd ICRC from Emulsion Chamber Experiments at Mt. Chacaltaya and Pamirs p 1-4 (SEE N94-256
Other
Cosmic Ray Showers, Energy Distribution, Hadrons, High Altitude, High Energy Interactions, Flux (Rate), Gamma Rays, High Altitude Environments, Space Observations (From Earth)
Scientific paper
A summary of the study on the global characteristics of very high energy cosmic-ray hadron interactions is presented. The study is carried out on the basis of 75 families recorded during the total of up to 1,400 sq m per year exposure at the Chacaltaya and the Pamir. The first striking encountered feature is those highest energy cosmic-ray families' wonderful variety in configurations. The second feature is the scantiness in frequency of the families at the Chacaltaya and Pamir altitudes. It will be convincing to assume that the higher energy portion of the constituent showers will reflect the characteristics of the family-generating main interaction directly. The scatter diagram of the number of hadrons against energy fraction of hadron component is shown. There are large differences between the observational and the simulational distributions which are of the same character as already noticed previously for the families with Efamily greater than or equal to 100 TeV. There exist families which are extremely rich in hadrons, in both multiplicity and energy fraction. They represent no other than the manifest indication that there exist exotic families with the characteristics similar to those of the 'Centauro-species'.
Baradzei T. L.
Borisov Anatoly S.
Cherdyntseva V. K.
Denisova G. V.
Dobrotin A. N.
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