Distribution of temperature coefficient density for muons in the atmosphere
To date, several dozens of new muon detectors have been built. When studying cosmic-ray intensity variations with these detectors, located deep in the atmosphere, it is necessary to calculate all characteristics, including the distribution of temperature coefficient density for muons in the atmosphe...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
INFRA-M
2017-12-01
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Series: | Solar-Terrestrial Physics |
Subjects: | |
Online Access: | https://naukaru.ru/ru/nauka/article/19715/view |