Measurement of the Flux of Ultra High Energy Cosmic Rays by the Stereo Technique
arXiv:0904.4500 · doi:10.1016/j.astropartphys.2009.06.001
Abstract
The High Resolution Fly's Eye experiment has measured the flux of ultrahigh energy cosmic rays using the stereoscopic air fluorescence technique. The HiRes experiment consists of two detectors that observe cosmic ray showers via the fluorescence light they emit. HiRes data can be analyzed in monocular mode, where each detector is treated separately, or in stereoscopic mode where they are considered together. Using the monocular mode the HiRes collaboration measured the cosmic ray spectrum and made the first observation of the Greisen-Zatsepin-Kuzmin cutoff. In this paper we present the cosmic ray spectrum measured by the stereoscopic technique. Good agreement is found with the monocular spectrum in all details.
20 pages, 10 figures
Cited by in corpus (18)
- Cosmogenic Neutrinos: parameter space and detectabilty from PeV to ZeV
- Star-forming galaxies as the origin of the IceCube PeV neutrinos
- Ultrahigh energy cosmic ray acceleration in newly born magnetars and their associated gravitational wave signatures
- Modeling the Spectral Energy Distribution of the radio galaxy IC310
- Neutrino, -ray and cosmic ray fluxes from the core of the closest radio galaxies
- A new limit on the Ultra-High-Energy Cosmic-Ray flux with the Westerbork Synthesis Radio Telescope
- Design and Initial Performance of the Prototype for the BEACON Instrument for Detection of Ultrahigh Energy Particles
- Comparing the energy spectra of ultra-high energy cosmic rays measured with EAS arrays
- On the synthesis of heavy nuclei in protomagnetar outflows and implications for ultra-high energy cosmic rays
- Systematic exploration of heavy element nucleosynthesis in protomagnetar outflows
- Measurement of the forward meson production rate in p-p collisions at =13 TeV with the LHCf-Arm2 detector
- Interpretation of measurements of the number of muons in extensive air shower experiments
- A Simple Parallelization Scheme for Extensive Air Shower Simulations
- A composition dependent energy scale and the determination of the cosmic ray primary mass in the ankle region
- Between the cosmic-ray `knee' and the `ankle': Contribution from star clusters
- Cosmic ray mass composition measurement in the energy range from eV to eV observed with the TALE hybrid detector
- High Energy Neutrinos and Cosmic Rays
- Implications of pc and kpc jet asymmetry to the cosmic ray acceleration