Physics
Scientific paper
Apr 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phrvd..77h3001h&link_type=abstract
Physical Review D, vol. 77, Issue 8, id. 083001
Physics
Extensive Air Showers, Observation And Data Reduction Techniques, Computer Modeling And Simulation, Cosmic Rays
Scientific paper
We have simulated more than 105 extensive air showers (EAS) by CORSIKA code, with a proton as the primary particle. The range of energy for primary particles was selected from 50 TeV to 5 PeV, with differential flux given by dN/dE∝E-2.7. Using the secondary charged particles produced of these EASs, we obtained the function dNsp(θ,X)/dθ, where Nsp(θ,X) is the number of secondary charged particles in EASs as a function of atmosphere depth, X, and zenith angle, θ. A sinθcosn(X)θ distribution was obtained for zenith angle distribution of the number of secondary charged particles, where power index, n(X), is a function of atmosphere depth, X. We obtained n(X)=3.02+0.003XlnX-8.28×10-9X3-1.35lnX. We have compared our results with the experimental data of various observatories.
Bahmanabadi Mahmoud
Ghomi Mehdi Khakian
Halataei M. H. S.
Samimi Jalal
No associations
LandOfFree
Simulation study on number of secondary particles in extensive air showers using CORSIKA code does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Simulation study on number of secondary particles in extensive air showers using CORSIKA code, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Simulation study on number of secondary particles in extensive air showers using CORSIKA code will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1697801