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On the halo events observed by mount fuji and mount kanbala emulsion chamber experiments
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | He, M. Kuang, H. H. Xue, Y. G. Lu, S. L. Huo, A. X. Ren, J. R. Su, S. Wang, C. R. Zhang, N. J. Wang, Y. X. |
| Copyright Year | 1985 |
| Description | The intensity of big gamma-ray families associated by halo is obtained from Mt. Fuji experiment (650 g/sq.cm. atmospheric depth) and Mt. Kanbala experiment (515 g/sq.cm.). The results are compared with Monte Carlo calculation based on several assumptions on interaction mechanisms and the primary cosmic ray composition. The results suggest more than 3 times lower proton abundance among primaries than that of 10 to the 12th to 10 to the 13th eV region within the framework of quasi-scaling model of multiple production. |
| File Size | 226320 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850027624 |
| Archival Resource Key | ark:/13960/t6f23tz6p |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Protons Energy Spectra Abundance Monte Carlo Method Nuclear Emulsions Cosmic Rays Gamma Rays Cosmic Ray Showers Halos Simulation Scaling Laws Models Detection Nuclear Interactions Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
