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...

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Bibliographic Details
Main Authors: Kuzmenko V.S., Yanchukovsky V.L.
Format: Article
Language:English
Published: INFRA-M 2017-12-01
Series:Solar-Terrestrial Physics
Subjects:
Online Access:https://naukaru.ru/ru/nauka/article/19715/view