Distribution of temperature coefficient density for muons in the atmosphere-Reference-Cited by-同舟云学术

Distribution of temperature coefficient density for muons in the atmosphere

Published:2017-12-29 Issue:4 Volume:3 Page:93-102
ISSN:2500-0535
Container-title:Solar-Terrestrial Physics
language:en
Short-container-title:

Author:

Кузьменко Василий¹,Kuzmenko Vasiliy²,Янчуковский Валерий¹,Yanchukovsky Valery²

Affiliation:

1. Институт нефтегазовой геологии и геофизики им. А.А. Трофимука СО РАН

2. A.A. Trofimuk Institute of Oil and Gas Geology and Geophysics SB RAS

Abstract

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 sea level and at various depths underground for different absorption ranges of primary protons and pions in the atmosphere.

Publisher

Infra-M Academic Publishing House

Subject

Space and Planetary Science,Atmospheric Science,Geophysics

Reference15 articles.

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