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Composition of primary cosmic rays near the bend from a study of hadrons in air showers at sea level
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Goodman, J. A. Berley, D. Tonwar, S. C. Ellsworth, R. W. Freudenreich, H. T. Mincer, A. I. Yodh, G. B. |
| Copyright Year | 1985 |
| Description | Data on hadrons in air showers arriving at sea level were studied to find sensitivity to primary cosmic ray composition. The rate of showers which satisfy minimum shower density and hadron energy requirements as well as the rate of showers containing hadrons delayed with respect to the electron shower front are compared to Monte Carlo simulations. The data on the rate of total triggers and delayed hadrons are compared to predicted rates for two models of primary composition. The data are consistent with models which require an increasing heavy nuclei fraction near 10 to the 15th power eV. The spectra which are consistent with the observed rate are also compared to the observed shower size spectrum at sea level and mountain level. |
| File Size | 273105 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850025746 |
| Archival Resource Key | ark:/13960/t7rn81s77 |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Hadrons Cosmic Ray Showers Ionizing Radiation Calorimeters Energy Spectra Energy Distribution Elementary Particles Electron Distribution Sea Level Monte Carlo Method Cosmic Rays Muons Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |