Manana Svanidze, Yuri Verbetsky, Ia Iashvili, Abesalom Iashvili, Alexi Gongadze, Levan Kakabadze, George Kapanadze, Edisher Tskhadadze, George Chonishvili
Published 2020-06-11Version 1
Extensive Air Showers (EAS) arrival direction distribution is studied by means of a 4-detector installation in Telavi (TEL array), which is a node of GELATICA net in Georgia. The description of EAS arrival zenith angle distribution within the spheric layer model of the atmosphere and exponential absorption of showers with the air path is used. It is shown that the variation of zenith angles upper cutoff boundary allows a stable estimation of showers absorption path.
Comments: PDF 9 pages A4; 9 figures; 15 references
Journal: Georgian Electronoc Scientific Jourmals (GESJ): Physics (2016) No.1(15) - 2740 pp.54-62 ISSN 1512-1461 ; http://gesj.internet-academy.org.ge/download.php?id=2740.pdf
On the angular distribution of extensive air showers
Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy
Calculation of rescaling factors and nuclear multiplication of muons in extensive air showers
![QR code for arXiv:2006.06509 [astro-ph.HE]](http://oss.arxitics.com/images/favicon.svg)