Distribution of temperature coefficient density for muons in the atmosphere


статья в журнале
Авторы: Kuzmenko V.S.   (ИНГГ СО РАН)   Yanchukovsky V.L.   (ИНГГ СО РАН)  
дата публикации: 2017
реферат:
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 atmosphere, taking into account their specific geometry. For this purpose, we calculate the density of temperature coefficients of muon intensity in the atmosphere at various zenith angles of detection at sea level and at various depths underground for different absorption ranges of primary protons and pions in the atmosphere.
первоисточник: Solar-Terrestrial Physics
том: 4
страницы: 93-102
ISBN:
ISSN:
внешние ссылки:
WoS   WoS (цитирование)
DOI  
РИНЦ SPIN  

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полный текст статьи

stp-2017-3-4-93