Computer Science
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7...52a&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 52-55 (SEE N85-35968 24-93)
Computer Science
Atmospheric Attenuation, Cerenkov Radiation, Cosmic Ray Showers, Electrons, Hadrons, Models, Distribution (Property), Energy Spectra, Parameterization, Scaling Laws, Simulation
Scientific paper
Comparison of experimental data on depth of extensive air showers (EAS) development maximum in the atmosphere, TM and path of absorption, lambda, in the lower atmosphere of EAS with fixed particle number in the energy region eV with the results of calculation show that these parameters are sensitive mainly to the inelastic interaction cross section and scaling violation in the fragmentation and pionization region. The data are explained in a unified manner within the framework of a model in which scaling is violated slightly in the fragmentation region and strongly in the pionization region at primary cosmic rays composition close to the normal one and a permanent increase of inelastic interaction cross section. It is shown that, while interpreting the experimental data, disregard of two methodical points causes a systematic shift in TM: (1) shower selection system; and (2) EAS electron lateral distribution when performing the calculations on basis of which the transfer is made from the Cerenkov pulse FWHM to the depth of shower maximum, T sub M.
Antonov Andrey Radoslavov
Galkin Vladimir I.
Hein L. A.
Ivanenko I. P.
Kanevsky B. L.
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