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Phenomenological characteristic of the electron component in gamma-quanta initiated showers
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Nikolsky, S. I. Ushev, S. Z. Stamenov, J. N. |
| Copyright Year | 1985 |
| Description | The phenomenological characteristics of the electron component in showers initiated by primary gamma-quanta were analyzed on the basis of the Tien Shan experimental data. It is shown that the lateral distribution of the electrons ion gamma-quanta initiated showers can be described with NKG - function with age parameters bar S equals 0, 76 plus or minus 0, 02, different from the same parameter for normal showers with the same size bar S equals 0, 85 plus or minus 0, 01. The lateral distribution of the correspondent electron energy flux in gamma-quanta initiated showers is steeper as in normal cosmic ray showers. |
| File Size | 138614 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850027721 |
| Archival Resource Key | ark:/13960/t49p7xk8w |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Protons Gamma Rays Cosmic Ray Showers Distribution Property Electrons Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
