INVESTIGATION OF THE AZIMUTHAL EFFECTS OF INITIAL GAMMA ENERGIES IN FAMILIES ΣEγ = 100 - 2000 TeV
( Pp. 138-142)

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Nuritdinov Khusnutdin kandidat fiz.-mat. nauk, zav. laboratoriey kosmicheskih luchey.
Physical-Technical Institute, «Physics-Sun». Uzbekistan Academy of sciences Absalyamova Ilmira Ildarovna mladshiy nauchnyy sotrudnik laboratorii kosmicheskih luchey
Physical-Technical Institute, «Physics-Sun». Uzbekistan Academy of sciences Kulakhmedov Nizamiddin Nuriddinovich starshiy nauchnyy sotrudnik laboratorii kosmicheskih luchey
Physical-Technical Institute, «Physics-Sun». Uzbekistan Academy of sciences Makhsudov Asatulla U. starshiy nauchnyy sotrudnik
Institute of Materials Science, SPA “Physics-Sun”, Academy of Science of Uzbekistan Shayakubov Diyor Bahtiyarovich mladshiy nauchnyy sotrudnik laboratorii kosmicheskih luchey
Physical-Technical Institute, «Physics-Sun». Uzbekistan Academy of sciences
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Abstract:
On the basis of experimental data «Pamir» in the field of ultrahigh-energy Eest = 1016 - 1017 eV, experiment and model MS0 considered parameters α - azimuthal anisotropy of the angular distributions of the secondary particles, and depending on the space-energy characteristics ER initial gamma-families formed during the interaction of protons and alpha particles of the primary cosmic rays (PCR) with air nuclei. In the experiment, an excess Δeksp = 0.10 ± 0.02 anisotropic initial γ-families with αin > 0.2 relative to the model. Mean value in the experiment appeared in the 1.6 times higher than in the model. In the region of small values of <500 TeV·mm setting is consistent among themselves, experiment and model and make small value ~ 0.10, and in the large > 500 TeV·mm observed a sharp increase in the experimental value of the parameter with the increase in performance. The values of one discussed above models remain essentially unchanged with the increase.
How to Cite:
Nuritdinov K.., Absalyamova I.I., Kulakhmedov N.N., Makhsudov A.U., Shayakubov D.B., (2016), INVESTIGATION OF THE AZIMUTHAL EFFECTS OF INITIAL GAMMA ENERGIES IN FAMILIES ΣEΓ = 100 - 2000 TEV. Computational Nanotechnology, 4: 138-142.
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Keywords:
primary cosmic rays, x-ray emulsion chambers, gamma family.