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Eas accompanied by gamma-families at mt. norikura and comparison with monte carlo simulation
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Torii, S. Sakata, M. Yamamoto, Y. Yuda, T. Saito, T. Shima, M. Kasahara, K. Hotta, N. |
| Copyright Year | 1985 |
| Description | The experimental data of extensive air showers (EAS) accompanied by gamma-families, with total energy greater than 10 TeV, were compared with a Monte Carlo simulation with a rising cross section proportional to E sup 0.04 for the p-air inelastic cross section. It is found that the absolute intensity of size spectrum of such EAS is strongly affected by the primary protons intensity at 10 to the 15th power approx. 10 to the 16th power eV region and the experimental size spectrum agrees with the simulated spectra for the p-poor primary composition better than the p-rich one. |
| File Size | 256284 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850027615 |
| Archival Resource Key | ark:/13960/t9b61fw1b |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Protons Gamma Rays Cosmic Ray Showers Particle Size Distribution Atmospheric Scattering Energy Distribution Monte Carlo Method Ionization Cross Sections Primary Cosmic Rays Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
