Temperature coefficients of muon intensity in the atmosphere

Using the results from continuous long-term observations, we obtain the distribution of temperature coefficient density for muons as registered for various zenith and azimuth angles and at different depths under the ground. Azimuthal anisotropy of the temperature effect is detected for atmospheric m...

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Bibliographic Details
Published inBulletin of the Russian Academy of Sciences. Physics Vol. 77; no. 5; pp. 566 - 568
Main Authors Yanchukovsky, V. L., Kuz’menko, V. S.
Format Journal Article
LanguageEnglish
Published Heidelberg Allerton Press, Inc 01.05.2013
Springer Nature B.V
Subjects
Hadrons
Heavy Ions
Muons
Nuclear Physics
Physics
Physics and Astronomy
Proceedings of the 32nd All-Russia Conference on Cosmic Rays
Temperature effects
Azimuthal Distribution
Azimuthal Anisotropy
Temperature Coefficient
Zenith Angle
Azimuth Angle
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Summary:Using the results from continuous long-term observations, we obtain the distribution of temperature coefficient density for muons as registered for various zenith and azimuth angles and at different depths under the ground. Azimuthal anisotropy of the temperature effect is detected for atmospheric muons.
ISSN:1062-8738
1934-9432
DOI:10.3103/S1062873813050535