Loading...
Please wait, while we are loading the content...
Similar Documents
Cosmic ray composition between 10 to the 15th power - 10 to the 17th power ev obtained by air shower experiments
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Muraki, Y. |
| Copyright Year | 1985 |
| Description | Based on the air shower data, the chemical composition of the primary cosmic rays in the energy range 10 to the 15th power - 10 to the 17th power eV was obtained. The method is based on a well known N sub e-N sub mu and N sub e-N sub gamma. The simulation is calibrated by the CERN SPS pp collider results. |
| File Size | 275613 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850025740 |
| Archival Resource Key | ark:/13960/t9c58gs0j |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Protons Iron Isotopes Cosmic Ray Showers Particle Interactions Energy Spectra Scattering Collision Parameters Chemical Composition Monte Carlo Method Collision Rates 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 |
