Analysis of the Arrival Directions of Ultrahigh Energy Cosmic Rays

Details Analysis of the Arrival Directions of Ultrahigh Energy Cosmic Rays Analysis of the Arrival Directions of Ultrahigh Energy Cosmic Rays

2007-05-17

arxiv.org/abs/0705.2466v1

Pre-conference ICRC 2007 proc., HE 1.4A, el.-disc

Astronomy and Astrophysics

Astrophysics

4 pages, 4 figures, PDF, a contributed paper presented to 30-th ICRC, Merida, Nexico, 2007

Scientific paper

The arrival directions of ultrahigh energy extensive air showers (EAS) by Yakutsk, AGASA and SUGAR array data are considered. For the first time, the maps of equal exposition of celestial sphere for the distribution of particles by AGASA and SUGAR array data have been constructed. The large-scale anisotropy of E>4.10^19 eV cosmic rays from the side of Input and Output of the Galaxy Local Arm by Yakutsk, AGASA and SUGAR array data has been detected. The problem of cosmic ray origin is discussed.

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