Its energy was so high it challenged scientists» assumptions about how high the energy of a cosmic ray could be and spawned the international Pierre
Auger Collaboration.
The new report by the Pierre
Auger Collaboration correlates in detail the signals in the water tanks with those from the telescopes.
He served as task leader for fluorescence detectors 1995 - 2001 and co-chair of
the Auger Collaboration Board 2001 - 2006.
The Pierre
Auger Collaboration has searched for the possible presence of photons with energies exceeding 1018 eV in the flux of cosmic rays arriving at Earth.
Related paper: Azimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger Observatory, Pierre
Auger Collaboration: A. Aab et al., Phys.
Related paper: Calibration of the Logarithmic - Periodic Dipole Antenna (LPDA) Radio Stations at the Pierre Auger Observatory using an Octocopter The Pierre
Auger Collaboration, 2017 JINST 12 T10005 [doi: 10.1088 / 1748-0221/12 / 10 / T10005][arXiv: 1702.01392]
The showers that
the Auger collaboration analyzed come from atmospheric cosmic - ray collisions that are 10 times higher in energy than the collisions produced at the LHC.
Related paper: Inferences on Mass Composition and Tests of Hadronic Interactions from 0.3 to 100 EeV using the water - Cherenkov Detectors of the Pierre Auger Observatory The Pierre
Auger Collaboration, Phys.
Related paper: Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory, A. Aab et al. (Pierre
Auger Collaboration), Phys.
Related paper: Ultrahigh - energy neutrino follow - up of gravitational wave events GW150914 and GW151226 with the Pierre Auger Observatory A. Aab et al. (Pierre
Auger Collaboration), Phys.
Use for commercial purposes shall require the approval by the Pierre
Auger Collaboration.
In November 2014 was recorded at the Pierre
Auger collaboration meeting material to make a 25 - min movie on cosmic rays, with a focus on the radio signal with AERA and CODALEMA / EXTASIS at Nancay, France.
This Video was realized by Aurelio Grillo, Pierre
Auger Collaboration, and Vincenzo Napolano, INFN Communication Office.
Related paper: Search for photons with energies above 1018 eV using the hybrid detector of the Pierre Auger Observatory The Pierre
Auger Collaboration, JCAP 04 (2017) 009 [http://dx.doi.org/10.1088/1475-7516/2017/04/009][arXiv: 1612.01517]
«It's the first clear experimental indication that the sources of these high - energy particles are located outside of our own galaxy, probably somewhere in the nearby universe,» says Karl - Heinz Kampert of the University of Wuppertal in Germany, a spokesperson for the Pierre
Auger Collaboration, which made the discovery.
The Pierre
Auger Collaboration.
Not exact matches
This section holds resources for the members of the Pierre
Auger Observatory
collaboration.
Progress towards understanding the analyses of mass composition made by the
Auger and Telescope Array
Collaborations
The 2014
Auger - sponsored Science Fair took place in the Assembly Building during the
collaboration meeting, November 19 - 21.
Jim Cronin had the vision and the force to put the international community in
collaboration to make alive
Auger Observatory.