[PDF] Top 20 Cosmic ray e± at high energy
Has 10000 "Cosmic ray e± at high energy" found on our website. Below are the top 20 most common "Cosmic ray e± at high energy".
Cosmic ray e± at high energy
... the widely used diffusion models for CR propagation have been successfully tested and calibrated along the years to fit observations of stable nuclei. These nuclei data in- clude a zoo of different elements, from primary ... See full document
5
Nucleus-nucleus interactions in very-high-energy cosmic ray experiments
... normal energy spectrum and composition of cosmic rays, and even the knee in the interval 1-10 PeV is ...very high energies of primary particles around 10 18 eV and ... See full document
13
Measurements of the proton-air cross section with high energy cosmic ray experiments
... The high energy models used to determine the value of K are ...the energy range of 10 ...the high energy models ...the high energy models used, the corresponding value of ... See full document
7
Correlation between the UHECRs measured by the Pierre Auger Observatory and Telescope Array and neutrino candidate events from IceCube
... ultra-high energy cosmic ray events measured by Telescope Array and the Pierre Auger Observatory and high-energy neutrino candidate events from ...ultra-high energy ... See full document
6
Constraining Dark Matter and Ultra-High Energy Cosmic Ray Sources with Fermi-LAT Diffuse Gamma Ray Background
... highest energy is still a subject of debate. All modern cosmic ray experiments extract information on the UHECR spectrum and composition from observations of extensive air showers (EAS), initiated by ... See full document
8
Abstract: The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a project dedicated to
... free cosmic-ray-detection application already while CRAYFIS is still in the beta ...the cosmic-rays ...secondary cosmic radiation, or possibly a particle of a local radiation, passes through ... See full document
6
ATLAS and ultra high energy cosmic ray physics
... the cosmic ray spectrum is due to the effect of some new hadronic physics threshold, where some 20% of the cosmic ray primary energy would need to be transferred to invisible ...a ... See full document
7
Ankle Phenomenon in the Cosmic Ray Energy Spectrum
... of cosmic ray pro- duction from AGN as well as in the process of universe ...in high energy cosmic ray showers and subsequently ... See full document
5
Neutrinos from colliding wind binaries: future prospects for PINGU and ORCA
... Cosmic ray energy spectra from stellar environments are believed to be of too low energy in order to explain the total flux of cosmic rays up to the knee: the observed cosmic ... See full document
5
Results and Perspectives of the Auger Engineering Radio Array
... for high-energy cosmic rays consisting of 153 autonomously-operating radio stations covering an area of 17 km 2 ...radiation energy of air showers was measured and compared with the accurate ... See full document
5
The future of the high energy cosmic ray detection: HERD
... excellent energy resolu- tion and long ...perform high statistics and precise measurements in the same energy range and beyond, to more than 10 TeV, of both spectral features and anisotropy, which ... See full document
7
Constraints on ultra-high-energy neutrino flux from radio observations of the Moon
... ultra-high- energy neutrinos and cosmic rays by using radio telescopes to search for short pulses from the ...or cosmic ray impinges on the Moon and interacts below the lunar ...the ... See full document
5
High energy cosmic ray anisotropies
... Multiple coincident muons or muon bundles observed in underground detectors are the remnants of air showers produced in the atmosphere by high energy cosmic ray protons and heavy nuclei.[r] ... See full document
186
Constraints on high energy interaction models from LHC and cosmic ray data
... of high energy hadronic interactions is of considerable importance for experimental studies at the Large Hadron Collider (LHC) and, especially, in high energy cosmic ray (CR) ... See full document
10
TAIGA - a hybrid array for high energy gamma astronomy and cosmic ray physics
... an energy, position, and direction of the EAS axis using the data of the wide-angle Cherenkov timing array TAIGA-HiSCORE (High Sensitivity COsmic Rays and gamma Explorer) ... See full document
8
Cosmic ray acceleration to ultrahigh energy in radio galaxies
... to a turbulent extragalactic field. The Jansson & Farrah [50] Galactic magnetic field model is then applied using the inbuilt lenses in CRPropa 3. The direction of deflec- tion is roughly towards the excess, although ... See full document
6
Results from NA61/SHINE
... Very High Energy Cosmic Ray Interactions, it is worth noting that although the di ff erent measurements are motivated by dif- ferent physics goals, all the hadron-nucleus and proton- proton ... See full document
7
TeV Blazars as the Sources of Ultra High Energy Cosmic Rays
... Ultra high energy cosmic rays (UHECRs) were defined as those cosmic rays with energies above 10 18 eV ...a cosmic ray primary with energy of 10 20 eV was reported [12], a ... See full document
12
Cosmic ray transport and anisotropies to high energies
... events is pretty much centered on Cen A also means that the linear bending integrates out to near zero; just the fluctua- tions produce an angular dispersion. If we accept the chemi- cal composition derived from Auger ... See full document
6
Development of the radio astronomical method of cosmic particle detection for extremely high-energy cosmic ray physics and neutrino astronomy
... particles in cascades induced by cosmic neutrinos. Then the radio emission of such cascades may be calculated. Some profiles for the total number of particles (electrons + positrons) as well as the charge excess ... See full document
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