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Results of investigation of muon fluxes of superhigh energy cosmic rays with x-ray emulsion chambers
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Mandritskaya, K. V. Ivanova, M. A. Rakobolskaya, I. V. Ivanenko, I. P. Zatsepin, G. T. Ilyina, N. P. Kuzmichev, L. A. Osipova, E. A. |
| Copyright Year | 1985 |
| Description | The overall data from the investigation of the cosmic ray muon flux in the range of zenith angles (0-90) deg within the energy range (3.5 to 5.0) TeV is presented. The exposure of large X-ray emulsion chambers underground was 1200 tons. year. The data were processe using the method which was applied in the experiment Pamir and differred from the earlier applied one. The obtained value of a slope power index of the differential energy spectrum of the global muon flux is =3.7 that corresponds to the slope of the pion generation differential spectrum, gamma sub PI = 2.75 + or - .04. The analysis of the muon zenith-angular distribution showed that the contribution of rapid generation muons in the total muon flux agree the best with the value .2% and less with .7% at a 90% reliability level. |
| File Size | 254074 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850027813 |
| Archival Resource Key | ark:/13960/t6d26t28t |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Gamma Rays Emulsions Flux Density Energy Spectra Angular Distribution High Energy Interactions Data Reduction 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 |
