[PDF] Top 20 Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory
Has 10000 "Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory" found on our website. Below are the top 20 most common "Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory".
Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory
... operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in ...to ... See full document
14
Measurement of the Muon Content of EAS With the Pierre Auger Observatory
... The Pierre Auger Observatory is a hybrid detector with the aim of studying the characteristics of the longitudinal and lateral profiles of ... See full document
6
Highlights from the Pierre Auger Observatory
... information of our spectrum measurement, it is possible that the cut-off region represents more a consequence of the source maximal acceleration energy (of the order ... See full document
9
Constraints on the origin of cosmic rays above $10^{18}$ eV from large scale anisotropy searches in data of the Pierre Auger Observatory
... several energy values covering the range 1 ≤ E/EeV ≤ 20 are shown in ...to the percent level, it is necessary to generate simulated event sets with at least ≃ 5 10 5 test ...number of ... See full document
16
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
... mic rays with energies above E = 5 × 10 18 eV arriving within an angular separation of approximately ...characterize the energy distributions inside these regions by two inde- pendent ... See full document
16
Ultrahigh Energy Neutrinos at the Pierre Auger Observatory
... High energy neutrinos can be detected with a variety of techniques [13, ...observed with arrays of detectors at ground level that are currently being used to measure extensive showers ... See full document
36
Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory
... A. The surface array of the Pierre Auger Observatory The Southern surface detector (SD) consists of 1600 Cherenkov water tanks ...altitude of 1400 m ... See full document
15
High-energy interactions at the Pierre Auger Observatory
... interaction of Ultra High Energy Cosmic Rays (UHECRs) with the atoms of the atmosphere can occur at center-of-mass energies that surpass 100 TeV, while ... See full document
7
Large-scale distribution of arrival directions of cosmic rays detected above 1018 ev at the pierre auger observatory
... distribution of arrival directions of UHECRs as a function of the energy is thus one important observable to provide key elements for understanding their origin in the EeV ... See full document
20
Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory
... For the subset of 50 events with a surface-detector reconstruction of the cosmic-ray energy, we have made a direct comparison with the associated ...compare ... See full document
20
Large Scale Distribution of Ultra High Energy Cosmic Rays Detected at the Pierre Auger Observatory With Zenith Angles up to 80°
... restrict the analysis to the first two harmonics k = 1, 2. The first harmonic coeffi- cients in right ascension and azimuth are enough to reconstruct the dipole in the hypothesis that ... See full document
26
Spectral Calibration of the Fluorescence Telescopes of the Pierre Auger Observatory
... The energy of the primary cosmic ray is a key measurable for the science of the observatory, and the FD measurement of the ... See full document
33
Upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the pierre auger observatory
... detection of ultrahigh energy (UHE) cosmic neu- trinos at EeV (1 EeV 10 18 eV) energies and above is a long-standing experimental ...to the universe [ 4 ], and provide an unique opportunity ... See full document
7
Improved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory
... flux of ultra-high energy cosmic rays (UHECRs) above ∼ 5 × 10 19 eV is known to be suppressed with respect to that extrapolated from lower ...in the UHECR spectrum [1, 2], ... See full document
14
Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory
... examples of the large-scale anisotropies expected from a Galactic CR component, we show in ...5 the direction of the dipole that would result for cosmic rays coming from ... See full document
16
Constraints and measurements of hadronic interactions in extensive air showers with the Pierre Auger Observatory
... goal of the Pierre Auger Observatory is to unveil the origin and nature of ...number of breakthroughs and some very important steps towards this goal have already ... See full document
9
Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory
... prediction of the background. We observe that the tail of the background distribution of F is consistent with an exponential ...to the distribution of F for ... See full document
16
Impact of Atmospheric Effects on the Energy Reconstruction of Air Showers Observed by the Surface Detectors of the Pierre Auger Observatory
... Variation of the atmospheric conditions affect the signals from the extended air shower (EAS) which can be detected at ground level with arrays of surface detectors, such as ... See full document
29
Azimuthal Asymmetry in the Risetime of the Surface Detector Signals of the Pierre Auger Observatory
... understanding of the properties and origin of cosmic rays with energies greater than 1 Joule ...for the origin of these particles must account for the ... See full document
16
Calibration of the logarithmic-periodic dipole antenna (LPDA) radio stations at the Pierre Auger Observatory using an octocopter
... calibration of a logarithmic periodic dipole antenna with a frequency coverage of 30 MHz to 80 MHz is ...part of a radio station sys- tem used for detection of cosmic ray ... See full document
39
temas relacionados