Cosmic Ray
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 ...
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Time Delays in Cosmic Ray Propagation
... Auger project cosmic ray arrival directions are correlated strongly with sources up to distances of 70 Mpc . For this to be true, or even if they are correlated with just the supergalactic plane, total ...
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Ionisation as indicator for cosmic ray acceleration
... the cosmic ray-induced ionisation rates, can be used as input for astrochemistry models in order to compute signa- tures indicating an enhanced ionisation rate, ...
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A solution to the cosmic ray anisotropy problem
... Aglietta, M., Alessandro, B., Antonioli, P., Arneodo, F., Bergam- asco, L., Bertaina, M., Bosio, A., Castellina, A., Castagnoli, C., Chiavassa, A., Cini Castagnoli, G., D’Ettorre Piazzoli, B., di Sci- ascio, G., ...
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Investigating the impacts of cosmic ray flux on tropospheric refractivity over nigeria
... of cosmic ray flux on tropospheric refractivity variations and its implication on radio communication in Nigeria ...while Cosmic rays data was downloaded from Mexico Cosmic ray ...of ...
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Cosmic Ray Interaction Models: an Overview
... to cosmic ray interaction models: a treatment of various hadron-nucleus and nucleus-nucleus interactions over a wide energy range, including the respective inelastic cross sections and particle production, ...
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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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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] ...
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Measurement of cosmic ray reconstruction efficiencies in the MicroBooNE LArTPC using a small external cosmic ray counter
... MuCS-triggered cosmic-ray muons with other nearby reconstructed tracks in the TPC, a selection requirement is placed on the maximum distance d max between the two points, (x reco , y reco , z reco ) and (x ...
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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 are developing a simple structure low cost fluores- cence detector for the next generation ultra-high energy cosmic ray observation named as Cosmic Ray Air Fluo- rescence Fresnel lens ...
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The cosmic ray anisotropy below 1015 eV
... the cosmic ray (CR) arrival direction distribution provides im- portant informations on the propagation mechanisms and on the identification of their ...
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Title: Unsupervised Learning on Cosmic Ray Daily Harmonic Variations
... Acknowledgement: The authors would like to thank Prof. S.P. Agrawal for his valuable suggestions and insights on the database as well as the daily harmonic variation parameters amplitude and phase, which have been used ...
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Cosmic ray transport and anisotropies to high energies
... the Cosmic Ray ...Galactic Cosmic Ray spectrum, its anisotropies, as well as the extragalactic ultra high energy Cosmic Rays, their chemical abundances and ...tic Cosmic Rays, a ...
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Nonlocal Models of Cosmic Ray Transport in the Galaxy
... Along with the isotropic model, the anisotropic diffusion model is used in local problems of galactic cosmic-ray transfer. This model was initially developed in theoretical studies of the motion of charged ...
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The COsmic ray Soil Moisture Interaction Code (COSMIC) for use in data assimilation
... assimilating cosmic-ray neutron intensity measured in air above the ...model, COsmic-ray Soil Moisture Interaction Code (COS- MIC), which is simple, physically based and analytic, and which, ...
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Connecting accelerator experiments and cosmic ray showers
... As a consequence of the indirect character of the measurement, detailed simulations of air showers are needed to extract information on the primary particle from shower observables. Indeed the cascade is initiated by a ...
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Ankle Phenomenon in the Cosmic Ray Energy Spectrum
... We assume that the target mass range for the search is from 8 TeV to 3 Pev. In particular, the 3 PeV target is of prime importance, since it is a starting point for the dis- covery of a new mass scale. Moreover, it ...
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Challenges for cosmic-ray experiments
... Composition from 1–100 EeV is the key to what is one of the most important open questions in cosmic- ray physics, namely, the cause of the apparent cutoff in the spectrum at 100 EeV. There are two ...
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Cosmic ray physics with the ARGO-YBJ experiment
... and cosmic ray physics below and around the knee of the primary energy spectrum (10 12 − 10 16 eV), where the transition from direct to indirect measurement techniques takes ...mic Ray Observatory of ...
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The power spectrum of cosmic ray arrival directions
... of cosmic ray diffusion we have to account for source terms of the initial dipole anisotropy in the form of a cosmic ray gradient ∇ ...
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