Loading...
Please wait, while we are loading the content...
Similar Documents
A new method to determine the chemical composition of the cosmic rays beyond 10 to the 15th power ev
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Muraki, Y. |
| Copyright Year | 1985 |
| Description | The chemical composition of primary cosmic rays beyond 10 to the 15th power eV could not be measured by the direct method. A more sensitive method to determine the chemical composition is proposed. The method was checked by simulation and compared with existing data on N sub e-N sub mu and N sub e-N sub gamma. |
| File Size | 23369 |
| Page Count | 1 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850025739 |
| Archival Resource Key | ark:/13960/t0ns5n14r |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Simulation Energy Spectra Comparison Spectral Signatures Chemical Composition Solar Cosmic Rays 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 |
