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Cosmic-ray intensity variations and temperature regime of the atmosphere
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Paper Abstract

Lifetime of muons is less than one-millionth of a second. Therefore, not all of them reach the level of their generation to the level of observations through the atmosphere. With the temperature changes occurs an extension or compression of the atmosphere, and hence the distance to the registration point of the particles. This is reflected in the change of the intensity recorded muons (temperature effect). Using the data of continuous observations of variations in cosmic ray intensity, obtained by using matrix muon telescope at Novosibirsk, there are temperature variations at different isobars in the atmosphere. The results obtained are compared with data from upper-air sounding.

Paper Details

Date Published: 18 December 2019
PDF: 5 pages
Proc. SPIE 11208, 25th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 112086T (18 December 2019); doi: 10.1117/12.2539301
Show Author Affiliations
Vasiliy S. Kuzmenko, Trofimuk Institute of Petroleum Geology and Geophysics (Russian Federation)
Valeriy L. Yanchukovsky, Trofimuk Institute of Petroleum Geology and Geophysics (Russian Federation)
Anastasiya Yu. Belinskaya, Trofimuk Institute of Petroleum Geology and Geophysics (Russian Federation)


Published in SPIE Proceedings Vol. 11208:
25th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics
Oleg A. Romanovskii; Gennadii G. Matvienko, Editor(s)

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