ijmpa˙paper International Journal of Modern Physics A c ○ World Scientific Publishing Company

The energy spectrum of primary cosmic rays with ultra–high energies based on the Yakutsk EAS Array data is presented. For the largest events values of S600 and axis coordinates have been obtained using revised lateral distribution function. The affect of the arrival time distribution at several axis...

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Bibliographic Details
Main Author: G. G Struchkov
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 2004
Subjects:
Yakutsk
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.254.4061
http://arxiv.org/pdf/astro-ph/0411685v1.pdf
Description
Summary:The energy spectrum of primary cosmic rays with ultra–high energies based on the Yakutsk EAS Array data is presented. For the largest events values of S600 and axis coordinates have been obtained using revised lateral distribution function. The affect of the arrival time distribution at several axis distance on estimated density for Yakutsk and AGASA is considered. 1.

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