scholarly journals The Search for Anisotropy in the Arrival Directions of Ultra-High Energy Cosmic Rays Observed by the High Resolution Fly's Eye Detector in Monocular Mode

2004 ◽  
Vol 136 ◽  
pp. 52-57
Author(s):  
Benjamin T. Stokes
2004 ◽  
Vol 610 (2) ◽  
pp. L73-L76 ◽  
Author(s):  
R. U. Abbasi ◽  
T. Abu-Zayyad ◽  
J. F. Amann ◽  
G. Archbold ◽  
R. Atkins ◽  
...  

2005 ◽  
Vol 622 (2) ◽  
pp. 910-926 ◽  
Author(s):  
R. U. Abbasi ◽  
T. Abu‐Zayyad ◽  
G. Archbold ◽  
R. Atkins ◽  
J. Bellido ◽  
...  

2011 ◽  
Vol 20 (supp02) ◽  
pp. 50-56
Author(s):  
◽  
PETER SCHIFFER

The Pierre Auger Observatory is the world's largest experiment for the measurement of ultra-high energy cosmic rays (UHECRs). These UHECRs are assumed to be to be charged particles, and thus are deflected in cosmic magnetic fields. Recent results of the Pierre Auger Observatory addressing the complex of energy ordering of the UHECRs arrival directions are reviewed in this contribution. So far no significant energy ordering has been observed.


2013 ◽  
Vol 28 (18) ◽  
pp. 1350075
Author(s):  
HANG BAE KIM

We study the anisotropy in the arrival directions of Pierre Auger Observatory (PAO) ultra-high-energy cosmic rays (UHECRs), using the point source correlational angular distance distribution (CADD). The result shows that the anisotropy is characterized by one prominent excess region and one void region. The excess region is located near the Centaurus A direction, supporting that the Centaurus A is a promising UHECR source. The void region near the south pole direction may be used to limit the diffuse isotropic background contribution.


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