On the possibility of investigation of the mass composition and energy spectra of primary cosmic ray (PCR) in the energy range from 10 exp 15 to 10 exp 17 eV using EAS data

Details On the possibility of investigation of the mass composition and energy spectra of primary cosmic ray (PCR) in the energy range from 10 exp 15 to 10 exp 17 eV using EAS data On the possibility of investigation of the mass composition and energy spectra of primary cosmic ray (PCR) in the energy range from 10 exp 15 to 10 exp 17 eV using EAS data

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ncimc..14..555c&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 14 C, Nov.-Dec. 1991, p. 555-568.

Physics

Condensed Matter

Statistical Mechanics

5

Energy Spectra, Particle Interactions, Primary Cosmic Rays, Radiation Spectra, Statistical Mechanics, Computerized Simulation, Monte Carlo Method, Multivariate Statistical Analysis, Particle Energy, Particle Mass, Probability Density Functions

Scientific paper

An analytical technique is developed which permits the derivation of the mass composition of primary cosmic radiation (PCR) by incorporating experimental data. Specific attention is given to utilizing nonparametric statistics for probability-density estimation and the quantitative comparison of multivariate distributions. Algorithms developed for experimental data handling are employed for the initial processing of events generated by means of the Monte Carlo method in order to check the present method. An experimental event can be selected efficiently that is initiated by primary protons and iron nuclei, and the energy spectrum of the incident protons and neutrons can be determined with the aid of the mutivariate data classification. The proposed method can facilitate the study of cosmic-ray interactions with the terrestrial atmosphere specifically for proton-nuclei and nuclei-nuclei interactions with energies of 10 exp 15-10 exp 17 eV.

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