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Temperature coefficients of muon intensity in the atmosphere

  • Proceedings of the 32nd All-Russia Conference on Cosmic Rays
  • Published:
Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

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.

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Authors and Affiliations

  1. Institute of Geophysics, Siberian Division, Russian Academy of Sciences, Novosibirsk, 630090, Russia

    V. L. Yanchukovsky & V. S. Kuz’menko

Authors
  1. V. L. Yanchukovsky
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  2. V. S. Kuz’menko
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Corresponding author

Correspondence to V. L. Yanchukovsky.

Additional information

Original Russian Text © V.L. Yanchukovsky, V.S. Kuz’menko, 2013, published in Izvestiya Rossiiskoi Akademii Nauk. Seriya Fizicheskaya, 2013, Vol. 77, No. 5, pp. 633–635.

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Yanchukovsky, V.L., Kuz’menko, V.S. Temperature coefficients of muon intensity in the atmosphere. Bull. Russ. Acad. Sci. Phys. 77, 566–568 (2013). https://doi.org/10.3103/S1062873813050535

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  • DOI: https://doi.org/10.3103/S1062873813050535

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