INFLUENCE OF PRIMARY COSMIC RADIATION MASS COMPOSITION ON THE ESTIMATION OF EAS ENERGY
Energy portion Eem/E0 transferred to EAS electron–photon component at E0 = 10 15 ± 10 19 eV was estimated by using of Čerenkov radiation data and charged particles data obtained at the Yakutsk array. The results are compared with the models for different energy dissipation into EAS electron– photon...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.254.9054 2023-05-15T18:45:25+02:00 INFLUENCE OF PRIMARY COSMIC RADIATION MASS COMPOSITION ON THE ESTIMATION OF EAS ENERGY S. P. Knurenko A. A. Ivanov V. A. Kolosov Z. E. Petrov I. Ye. Sleptsov G. G. Struchkov The Pennsylvania State University CiteSeerX Archives 2005 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.254.9054 http://arxiv.org/pdf/astro-ph/0411682v2.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.254.9054 http://arxiv.org/pdf/astro-ph/0411682v2.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/0411682v2.pdf Cosmic Rays Extensive Air Showers Mass Composition text 2005 ftciteseerx 2016-01-07T19:53:31Z Energy portion Eem/E0 transferred to EAS electron–photon component at E0 = 10 15 ± 10 19 eV was estimated by using of Čerenkov radiation data and charged particles data obtained at the Yakutsk array. The results are compared with the models for different energy dissipation into EAS electron– photon component and with calculations for different primary nuclei. In the energy intervals 10 15 ± 10 16 eV and 10 18 ±10 19 eV Eem/E0 is equal to (77 ±2) and (88 ±2) % respectively, that doesn’t contradict with mixed composition of primary particles for the first energy interval and the proton composition for the second one. Text Yakutsk Unknown Yakutsk |
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English |
topic |
Cosmic Rays Extensive Air Showers Mass Composition |
spellingShingle |
Cosmic Rays Extensive Air Showers Mass Composition S. P. Knurenko A. A. Ivanov V. A. Kolosov Z. E. Petrov I. Ye. Sleptsov G. G. Struchkov INFLUENCE OF PRIMARY COSMIC RADIATION MASS COMPOSITION ON THE ESTIMATION OF EAS ENERGY |
topic_facet |
Cosmic Rays Extensive Air Showers Mass Composition |
description |
Energy portion Eem/E0 transferred to EAS electron–photon component at E0 = 10 15 ± 10 19 eV was estimated by using of Čerenkov radiation data and charged particles data obtained at the Yakutsk array. The results are compared with the models for different energy dissipation into EAS electron– photon component and with calculations for different primary nuclei. In the energy intervals 10 15 ± 10 16 eV and 10 18 ±10 19 eV Eem/E0 is equal to (77 ±2) and (88 ±2) % respectively, that doesn’t contradict with mixed composition of primary particles for the first energy interval and the proton composition for the second one. |
author2 |
The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
S. P. Knurenko A. A. Ivanov V. A. Kolosov Z. E. Petrov I. Ye. Sleptsov G. G. Struchkov |
author_facet |
S. P. Knurenko A. A. Ivanov V. A. Kolosov Z. E. Petrov I. Ye. Sleptsov G. G. Struchkov |
author_sort |
S. P. Knurenko |
title |
INFLUENCE OF PRIMARY COSMIC RADIATION MASS COMPOSITION ON THE ESTIMATION OF EAS ENERGY |
title_short |
INFLUENCE OF PRIMARY COSMIC RADIATION MASS COMPOSITION ON THE ESTIMATION OF EAS ENERGY |
title_full |
INFLUENCE OF PRIMARY COSMIC RADIATION MASS COMPOSITION ON THE ESTIMATION OF EAS ENERGY |
title_fullStr |
INFLUENCE OF PRIMARY COSMIC RADIATION MASS COMPOSITION ON THE ESTIMATION OF EAS ENERGY |
title_full_unstemmed |
INFLUENCE OF PRIMARY COSMIC RADIATION MASS COMPOSITION ON THE ESTIMATION OF EAS ENERGY |
title_sort |
influence of primary cosmic radiation mass composition on the estimation of eas energy |
publishDate |
2005 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.254.9054 http://arxiv.org/pdf/astro-ph/0411682v2.pdf |
geographic |
Yakutsk |
geographic_facet |
Yakutsk |
genre |
Yakutsk |
genre_facet |
Yakutsk |
op_source |
http://arxiv.org/pdf/astro-ph/0411682v2.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.254.9054 http://arxiv.org/pdf/astro-ph/0411682v2.pdf |
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Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766236473918488576 |