Phenomenological characteristic of the electron component in gamma-quanta initiated showers

Details Phenomenological characteristic of the electron component in gamma-quanta initiated showers Phenomenological characteristic of the electron component in gamma-quanta initiated showers

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7..247n&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 247-250 (SEE N85-35968 24-93)

Mathematics

Logic

Cosmic Ray Showers, Electrons, Gamma Rays, Distribution (Property), Protons

Scientific paper

The phenomenological characteristics of the electron component in showers initiated by primary gamma-quanta were analyzed on the basis of the Tien Shan experimental data. It is shown that the lateral distribution of the electrons ion gamma-quanta initiated showers can be described with NKG - function with age parameters bar S equals 0, 76 plus or minus 0, 02, different from the same parameter for normal showers with the same size bar S equals 0, 85 plus or minus 0, 01. The lateral distribution of the correspondent electron energy flux in gamma-quanta initiated showers is steeper as in normal cosmic ray showers.

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