cosmic ray experiments
Measurements of the proton-air cross section with high energy cosmic ray experiments
... from cosmic ray experiments like Fly’s Eye [11], Akeno [15], HiRes [18], and Auger [13], together with accelerator pp and ¯pp cross section measurement [27], and the recent result from the LHC, by ...
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Challenges for cosmic-ray experiments
... of cosmic rays produced and they would be confined in the host galaxy sufficiently long that most protons would interact (calorimetric ...of cosmic-ray induced neutrinos and photons must have a hard ...
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Nucleus-nucleus interactions in very-high-energy cosmic ray experiments
... of cosmic rays are performed in space, at higher layers of the atmosphere, on the mountains, on the Earth's surface (near sea level), underground (under water and under ...
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Proton-air and proton-proton cross sections
... cise cosmic ray data can be directly sensitive to hadronic cross ...of cosmic ray experiments, at ultra-high energies, it became feasible to measure the longitudinal fluctuations of air ...
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NEEDS for LHC experiment planning from results of very high energy cosmic ray Investigations (NEEDS-2)
... of cosmic ray ...of cosmic ray experiments at LHC energies are ...LHC experiments from investigations of pp-interactions to investigations of nucleus-nucleus interactions is ...
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Detection of ultra-high energy cosmic ray air showers by Cosmic Ray Air Fluorescence Fresnel lens Telescope for next generation
... We also developed detector simulation to understand our optics, to optimize the configuration of the detector, and develop the analysis method. The actual detector config- uration of CRAFFT is considered in the ...
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Investigating the Apparent Link between Cosmic Ray Muon Flux, Sudden Stratospheric Warming and Dry Season Rainfall over Jamaica
... Cosmic ray Muons are sub-atomicparticles formed when cosmic radiation inte- ract with molecules within the Earth’s ...to cosmic-ray Muon ...
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The influence of the sidereal cosmic ray anisotropies originated on the tail and nose boundaries of the heliomagnetosphere (HMS) upon the solar cosmic ray anisotropy produced inside the HMS
... of cosmic rays observed with the neutron monitors and the muon tele- scopes on the ground does not coincide with that expected from the diffusion-convection ...
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Cosmic x ray surveys
... The total 2-8 keV count rates obtained from the analysis were in good agreement between the two flights,, and the ratio of 2-5 keV/5-8 keV counts in flight II indicated a source temperat[r] ...
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Cosmic ray modulation in the heliosphere
... 1 fi+1,j,kfi-1,j,k gri,j,k = f tj,k rt+i ri-1 The integral value of the radial gradient between two rigidity values was calculated using the same central difference approximation, except[r] ...
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Measurement of ultra-high energy cosmic rays: An experimental summary and prospects
... eV cosmic ray proton colliding with a proton target at ...forward experiments at the LHC are particularly ...for cosmic ray related ...
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Cosmic x ray surveys
... in the case of Sco XR-1, the large optical depth at optical and radio frequencies and the high temperatures of the thermal plasma implies significant electron scattering accompanied by d[r] ...
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Measurement of cosmic ray reconstruction efficiencies in the MicroBooNE LArTPC using a small external cosmic ray counter
... study cosmic rays corresponding to bins with larger σ in more detail and two contributing factors that lead to non-uniformities: regions of the detector with unresponsive wires and highly inclined ...the ...
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Time Delays in Cosmic Ray Propagation
... It is usual to think of CR acceleration being through diffusive shock acceleration. This process is rather slow [9] and requires a stable shock front, or at least a stable magnetic containment region. Source lifetimes ...
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Cosmic Ray Interaction Models: an Overview
... energy cosmic rays (CR) are traditionally performed using the so-called extensive air shower (EAS) techniques: the properties of the primary CR particles are reconstructed from measured characteristics of ...
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Cosmic Ray Mass Measurements with LOFAR
... indicate 1σ statistical uncertainties and the shaded region shows the systematic uncertainty. The values are in agreement with other experiments using different techniques (fluorescence detection and non-imaging ...
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Cosmic ray e± at high energy
... We show that recent measurements of the total e ± flux at E 3 TeV are in good agreement with the predicted flux of secondary e ± , that would be obtained if radiative energy losses duri[r] ...
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The distribution of cosmic ray neutrons in the atmosphere
... xLi iiCalibration of neutron density detectors 175 iiiNeutron density measurements in flight DN3 179 ivNormalisation to measurements by Miles 1964 180 v Comparison with the results of Li[r] ...
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Diurnal and transient cosmic ray variations
... S.E", FOPJIUSK 1969 , "Variation with a period of two solar cycles in the Cosmic-Ray diurnal anisotropy and the superposed variations correlated with magnetic activity", J.. "Monte Carlo[r] ...
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