Cosmic Rays with Energy Above 10^{17} ev

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 Authors: Egorova, V P, Glushkov, A V, Ivanov, A A, Knurenko, S P, Kolosov, V A, Krasilnikov, A D, Makarov, I T, Mikhailov, A A, Olzoyev, V V, Pravdin, M I, Sabourov, A V, Sleptsov, I Ye, Struchkov, G G
Language:English
Published: 2004
Subjects:
Astrophysics and Astronomy
Yakutsk
Online Access:http://cds.cern.ch/record/807483
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.

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