Email this article Cosmic ray spectrum measured by the PRISMA-32 setup
- Authors: 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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Affiliations:
- National Research Nuclear University “MEPhI”
- Institute for Nuclear Research
- Issue: Vol 44, No 10 (2017)
- Pages: 295-297
- Section: Article
- URL: https://journals.rcsi.science/1068-3356/article/view/228469
- DOI: https://doi.org/10.3103/S1068335617100050
- ID: 228469
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Abstract
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.
About the authors
K. O. Yurin
National Research Nuclear University “MEPhI”
Author for correspondence.
Email: KOYurin@mephi.ru
Russian Federation, Kashirskoe sh. 31, Moscow, 115409
F. A. Bogdanov
National Research Nuclear University “MEPhI”
Email: KOYurin@mephi.ru
Russian Federation, Kashirskoe sh. 31, Moscow, 115409
D. M. Gromushkin
National Research Nuclear University “MEPhI”
Email: KOYurin@mephi.ru
Russian Federation, Kashirskoe sh. 31, Moscow, 115409
Yu. V. Sten’kin
National Research Nuclear University “MEPhI”; Institute for Nuclear Research
Email: KOYurin@mephi.ru
Russian Federation, Kashirskoe sh. 31, Moscow, 115409; pr. 60-letiya Octyabrya 7a, Moscow, 117312
O. B. Shchegolev
Institute for Nuclear Research
Email: KOYurin@mephi.ru
Russian Federation, pr. 60-letiya Octyabrya 7a, Moscow, 117312
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