Anisotropy of Arrival Directions of E0 > 8 x 10**18 eV Cosmic Rays and Cosmic Microwave Background
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 v...
| Main Author: | |
|---|---|
| Format: | Text |
| Language: | unknown |
| Published: |
arXiv
2012
|
| Subjects: | |
| Online Access: | https://dx.doi.org/10.48550/arxiv.1202.5345 https://arxiv.org/abs/1202.5345 |
| Summary: | 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. : 4 pages, 2 figures |
|---|