26-28 September 2013
Union South, UW-Madison
US/Central timezone

Large-Scale Distribution of Arrival Directions of Cosmic Rays Detected at the Pierre Auger Observatory Above ~10 PeV

26 Sep 2013, 11:50
20m
Northwoods (Union South, UW-Madison)

Northwoods

Union South, UW-Madison

1308 West Dayton Street, Madison, WI 53706

Speaker

Dr Olivier Deligny (CNRS/IN2P3 - IPN Orsay)

Description

Harmonic analyses dedicated to searches for large-scale anisotropies in both right ascension and declination distributions of cosmic rays detected above ~10 PeV at the Pierre Auger Observatory are presented. Though additional statistics is still needed to characterize unambiguously the patterns as a function of the energy due to their relatively low dipole and quadrupole amplitudes, the focus is given to the few current hints that may be indicative of the presence of a structure at large scale over a wide energy range. On the other hand, the constraints on the production of cosmic rays provided by the upper limits obtained on the dipole and quadrupole amplitudes in the EeV energy range are discussed.

Primary author

Dr Olivier Deligny (CNRS/IN2P3 - IPN Orsay)

Presentation Materials