Cosmic Rays with Energy Above 10^{17} ev

A.A. Ivanov; A.A. Mikhailov; A.D. Krasilnikov; A.V. Glushkov; A.V. Sabourov; G.G Struchkov; I.T. Makarov; I.Ye. Sleptsov; M.I. Pravdin; S.P. Knurenko

arxiv: astro-ph/0411685 · v1 · submitted 2004-11-25 · 🌌 astro-ph

Cosmic Rays with Energy Above 10¹⁷ ev

V.P. Egorova , A.V. Glushkov , A.A. Ivanov , S.P. Knurenko , V.A. Kolosov , A.D. Krasilnikov , I.T. Makarov , A.A. Mikhailov

show 5 more authors

V.V. Olzoyev M.I. Pravdin A.V. Sabourov I.Ye. Sleptsov G.G Struchkov

This is my paper

classification 🌌 astro-ph

keywords axiscosmicdistributionenergyraysyakutskaboveaffect

0 comments

read the original abstract

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.

This paper has not been read by Pith yet.

Cosmic Rays with Energy Above 10¹⁷ ev

discussion (0)