Anisotropy of Arrival Directions of E0 > 8 x 10**18 eV Cosmic Rays and Cosmic Microwave Background

Details Anisotropy of Arrival Directions of E0 > 8 x 10**18 eV Cosmic Rays and Cosmic Microwave Background Anisotropy of Arrival Directions of E0 > 8 x 10**18 eV Cosmic Rays and Cosmic Microwave Background

2012-02-23

arxiv.org/abs/1202.5345v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

4 pages, 2 figures

Scientific paper

10.1134/S1063778808080103

Results are presented that were obtained by analysing the arrival directions of E0 > 8x10**18 eV primary cosmic rays recorded at the Yakutsk array over the period between 1974 and 2003 and at the SUGAR array (Australia). The greatest primary cosmic ray flux is shown to arrive from the region of visible intersection of the planes of the Galaxy and the Supergalaxy (local supercluster of galaxies) at a galactic longitude of about 137 degres. On a global scale, the lowest temperature of the cosmic microwave background is typical of this region.

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