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Muon groups and primary composition at 10 to the 13th power to 10 to the 15th power ev
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Mihelev, A. R. Padey, V. A. Suvorova, O. V. Chudakov, A. E. Voevodsky, A. V. Budko, E. V. Dogujaev, V. A. Petkov, V. A. Striganov, P. S. |
| Copyright Year | 1985 |
| Description | The data on muon groups observed at Baksan underground scintillation telescope is analyzed. In this analysis we compare the experimental data with calulations, based on a superposition model in order to obtain the effective atomic number of primary cosmic rays in the energy range 10 to the 13th power to 10 to the 15th power eV. |
| File Size | 215095 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850027761 |
| Archival Resource Key | ark:/13960/t01z92z30 |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Scintillation Counters Simulation Energy Spectra Monte Carlo Method Distribution Functions Nucleon-nucleon Interactions Primary Cosmic Rays Muons Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
