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Measuring the energy spectrum of primary cosmic rays with the yakutsk eas array
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Khristiansen, G. B. |
| Copyright Year | 1986 |
| Description | The Yakutsk Extensive Air Showers (EAS) array was designed for detecting the showers generated by the 10 to the 47th power to 10 to the 20th power eV primary cosmic rays and consists of numerous electron, muon, and Cerenkov light detectors arranged on a 20 sq km area terrain. The array is featured by the feasibility to detect the EAS-produced Cerenkov light, hence, as will be shown, to find the mean energy of the primary particles generating an ensemble of EAS of given size. Date collected is discussed. |
| File Size | 586770 |
| Page Count | 11 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19860022039 |
| Archival Resource Key | ark:/13960/t5r83771d |
| Language | English |
| Publisher Date | 1986-02-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Energy Spectra Light Scattering Cerenkov Counters Distortion Particle Density Concentration Monte Carlo Method Gamma Ray Bursts Cosmic Rays Distribution Functions 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 |
