Distribution of temperature coefficient density for muons in the atmosphere

Василий Кузьменко, Vasiliy Kuzmenko, Валерий Янчуковский, Valery Yanchukovsky
2017 Solar-Terrestrial Physics  
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 character-istics, including the distribution of temperature coeffi-cient 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
more » ... es of detection at sea level and at various depths underground for different absorption ranges of primary protons and pions in the atmosphere.
doi:10.12737/stp-34201710 fatcat:sa6yn5csk5daxewzizd6xd7l7m