Enviar artigo por via de e-mail Cosmic ray spectrum measured by the PRISMA-32 setup
- Autores: Yurin K.O.1, Bogdanov F.A.1, Gromushkin D.M.1, Sten’kin Y.V.1,2, Shchegolev O.B.2
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Afiliações:
- National Research Nuclear University “MEPhI”
- Institute for Nuclear Research
- Edição: Volume 44, Nº 10 (2017)
- Páginas: 295-297
- Seção: Article
- URL: https://journals.rcsi.science/1068-3356/article/view/228469
- DOI: https://doi.org/10.3103/S1068335617100050
- ID: 228469
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Resumo
The results of measurements of the spectrum of extensive air showers (EASs) by the number of neutrons detected by the PRISMA-32 setup are presented. The neutron component is formed during the interaction of high-energy shower hadrons with nuclei of atmospheric and Earth’s surface atoms. The PRISMA-32 setup consists of 32 en-detectors and operates in the continuous mode for about 5 years.
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Sobre autores
K. Yurin
National Research Nuclear University “MEPhI”
Autor responsável pela correspondência
Email: KOYurin@mephi.ru
Rússia, Kashirskoe sh. 31, Moscow, 115409
F. Bogdanov
National Research Nuclear University “MEPhI”
Email: KOYurin@mephi.ru
Rússia, Kashirskoe sh. 31, Moscow, 115409
D. Gromushkin
National Research Nuclear University “MEPhI”
Email: KOYurin@mephi.ru
Rússia, Kashirskoe sh. 31, Moscow, 115409
Yu. Sten’kin
National Research Nuclear University “MEPhI”; Institute for Nuclear Research
Email: KOYurin@mephi.ru
Rússia, Kashirskoe sh. 31, Moscow, 115409; pr. 60-letiya Octyabrya 7a, Moscow, 117312
O. Shchegolev
Institute for Nuclear Research
Email: KOYurin@mephi.ru
Rússia, pr. 60-letiya Octyabrya 7a, Moscow, 117312
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