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On the determination of the depth of eas development maximum using the lateral distribution of cerenkov light at distances 150 m from eas axis
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Alimov, T. Kakhkharov, M. Tashpulatov, R. Khristiansen, G. B. Kalmykov, N. N. Prosin, V. V. Aliev, N. Makhmudov, B. M. Rakhimova, N. |
| Copyright Year | 1985 |
| Description | The Samarkand extensive air showers (EAS) array was used to measure the mean and individual lateral distribution functions (LDF) of EAS Cerenkov light. The analysis of the individual parameters b showed that the mean depth of EAS maximum and the variance of the depth distribution of maxima of EAS with energies of approx. 2x10 to the 15th power eV can properly be described in terms of Kaidalov-Martirosyan quark-gluon string model (QGSM). |
| File Size | 182678 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850027706 |
| Archival Resource Key | ark:/13960/t8vb31c4m |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Cosmic Ray Showers Light Visible Radiation Flux Density Energy Spectra Cerenkov Radiation Radiation Counters Flux Rate Cosmic Rays Distribution Functions Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |