Cosmic ray spectrum measured by the PRISMA-32 setup


Дәйексөз келтіру

Толық мәтін

Ашық рұқсат Ашық рұқсат
Рұқсат жабық Рұқсат берілді
Рұқсат жабық Тек жазылушылар үшін

Аннотация

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.

Авторлар туралы

K. Yurin

National Research Nuclear University “MEPhI”

Хат алмасуға жауапты Автор.
Email: KOYurin@mephi.ru
Ресей, Kashirskoe sh. 31, Moscow, 115409

F. Bogdanov

National Research Nuclear University “MEPhI”

Email: KOYurin@mephi.ru
Ресей, Kashirskoe sh. 31, Moscow, 115409

D. Gromushkin

National Research Nuclear University “MEPhI”

Email: KOYurin@mephi.ru
Ресей, Kashirskoe sh. 31, Moscow, 115409

Yu. Sten’kin

National Research Nuclear University “MEPhI”; Institute for Nuclear Research

Email: KOYurin@mephi.ru
Ресей, Kashirskoe sh. 31, Moscow, 115409; pr. 60-letiya Octyabrya 7a, Moscow, 117312

O. Shchegolev

Institute for Nuclear Research

Email: KOYurin@mephi.ru
Ресей, pr. 60-letiya Octyabrya 7a, Moscow, 117312

Қосымша файлдар

Қосымша файлдар
Әрекет
1. JATS XML

© Allerton Press, Inc., 2017