Results 121 to 130 of about 19,659 (274)

Hybrid Performance of the Pierre Auger Observatory [PDF]

open access: yes, 2007
A key feature of the Pierre Auger Observatory is its hybrid design, in which ultra high energy cosmic rays are detected simultaneously by fluorescence telescopes and a ground array.
Dawson, B. R.
core   +1 more source

Neutrino probe of cosmic ray astrophysics and new physics at sub-fermi distances

open access: yes, 2009
We show that if the evolution of cosmic ray sources follows that of active galactic nuclei, the upper limit on the diffuse flux of tau neutrinos from the Pierre Auger Observatory marginally constrains the proton fraction at the end of the energy spectrum.
Anchordoqui, Luis A.
core   +1 more source

The Lidar System of the Pierre Auger Observatory [PDF]

open access: yes, 2006
The Pierre Auger Observatory in Malargue, Argentina, is designed to study the origin of ultrahigh energy cosmic rays with energies above 10^18 eV. The energy calibration of the detector is based on a system of four air fluorescence detectors.
BenZvi, S Y   +29 more
core   +2 more sources

Results and Perspectives of the Auger Engineering Radio Array [PDF]

open access: yes, 2016
The Auger Engineering Radio Array (AERA) is an extension of the Pierre Auger Cosmic-Ray Observatory. It is used to detect radio emission from extensive air showers with energies beyond $10^{17}~$eV in the $30 - 80~$MHz frequency band.
Glaser, Christian
core   +2 more sources

Experimental aspects of cosmic rays [PDF]

open access: yes, 2006
High-energy cosmic rays are detected as extensive air showers, and properties of the primary cosmic rays are deduced from measurements of those air showers.
Sommers, P
core   +1 more source

Welcome to Pierre Auger Observatory

open access: yes, 2022
Presentation at the REINFORCE International Training Course 2022.
openaire   +1 more source

Measurements of the muonic component of air showers at the Pierre Auger Observatory

open access: yesEPJ Web of Conferences, 2013
Several methods have been developed by the Pierre Auger Collaboration to estimate the muon content of air showers from ultra-high energy cosmic rays.
Allen Jeff
doaj   +1 more source

Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory [PDF]

open access: yes, 2019
Neutrinos with energies above 10(17) eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well
A. Aab   +390 more
semanticscholar   +1 more source

Recent results from the Pierre Auger Observatory on the mass composition and hadronic interactions of ultra-high energy cosmic rays

open access: yesEPJ Web of Conferences, 2017
Recent results on the mass composition and hadronic interactions of ultra-high energy cosmic rays (UHECR) obtained at the Pierre Auger Observatory are reviewed.
Yushkov Alexey
doaj   +2 more sources

Report of the Working Group on the Composition of Ultra High Energy Cosmic Rays

open access: yes, 2015
For the first time a proper comparison of the average depth of shower maximum ($X_{\rm max}$) published by the Pierre Auger and Telescope Array Observatories is presented.
Abbasi, R.   +12 more
core   +1 more source

Home - About - Disclaimer - Privacy