Add to ORKGMore than 3000 extensive air showers with energies above 1018 eV were observed in stereo mode by the HiRes stereo nitrogen fluorescence detector. Energy and Xmax were determined for each event. The proton-air inelastic cross-section was measured using the Xmax distribution and a newly developed deconvolution method. The results are found to be in good agreement with previous measurements by AKENO and Fly's Eye
Anomalous extensive air showers have yet to be detected by cosmic ray observatories. Fluorescence de...
In this work the results of p-air cross section measurements with the ARGO-YBJ experiment are report...
A precise measurement of the energy is essential for the study of ultra-high energy cosmic rays. Bas...
The distribution of the maxima of high energy cosmic ray induced extensive air showers in the atmosp...
In this paper, we will discuss the prospects of deducing the proton-air cross section from fluoresce...
Since the discovery of cosmic rays about one century ago, there have been two main approaches in the...
Ultra high energy cosmic rays provide the highest known energy source in the universe to measure pro...
We report a measurement of the proton-air cross section for particle production at the center-of-mas...
One of the most promising approaches to determine the energy spectrum and composition of cosmic rays...
In this work we are reporting on the measurement of the proton-air inelastic cross section sigma(ine...
Ultrahigh energy cosmic rays provide the highest known energy source in the Universe to measure prot...
Ultrahigh energy cosmic rays provide the highest known energy source in the Universe to measure prot...
The proton-air inelastic cross section (σp-airinel) is measured at s≈2TeV at the EAS-TOP extensive a...
The proton-air inelastic cross section (σp-airinel) is measured at √s≈2 TeV at the EAS-TOP extensiv...
The nitrogen fluorescence induced in air is used to detect ultra-high energy cosmic rays and to meas...
Anomalous extensive air showers have yet to be detected by cosmic ray observatories. Fluorescence de...
In this work the results of p-air cross section measurements with the ARGO-YBJ experiment are report...
A precise measurement of the energy is essential for the study of ultra-high energy cosmic rays. Bas...
The distribution of the maxima of high energy cosmic ray induced extensive air showers in the atmosp...
In this paper, we will discuss the prospects of deducing the proton-air cross section from fluoresce...
Since the discovery of cosmic rays about one century ago, there have been two main approaches in the...
Ultra high energy cosmic rays provide the highest known energy source in the universe to measure pro...
We report a measurement of the proton-air cross section for particle production at the center-of-mas...
One of the most promising approaches to determine the energy spectrum and composition of cosmic rays...
In this work we are reporting on the measurement of the proton-air inelastic cross section sigma(ine...
Ultrahigh energy cosmic rays provide the highest known energy source in the Universe to measure prot...
Ultrahigh energy cosmic rays provide the highest known energy source in the Universe to measure prot...
The proton-air inelastic cross section (σp-airinel) is measured at s≈2TeV at the EAS-TOP extensive a...
The proton-air inelastic cross section (σp-airinel) is measured at √s≈2 TeV at the EAS-TOP extensiv...
The nitrogen fluorescence induced in air is used to detect ultra-high energy cosmic rays and to meas...
Anomalous extensive air showers have yet to be detected by cosmic ray observatories. Fluorescence de...
In this work the results of p-air cross section measurements with the ARGO-YBJ experiment are report...
A precise measurement of the energy is essential for the study of ultra-high energy cosmic rays. Bas...