The mean-mass temperature and the spectrographic method of studying cosmic ray variations

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Cosmic Rays, Mesons, Muons, Spectroscopic Analysis, Temperature Measurement, Atmospheric Temperature, Integral Equations, Neutrons, Particle Energy, Temperature Distribution

Scientific paper

The potential of spectrography in the study of cosmic ray variations can be improved by using data on such unstable components (characterized by appreciable temperature effects) as the muon component, in addition to data on the neutron component. In the present paper, a method of determining temperature variations in the meson component of cosmic rays is examined. It is based on the use of spectrographic recordings of the neutron component at 435, 2000, and 300 meters above sea level and of hard muons at the 435-m level. It is shown that owing to the specifics of the density temperature coefficient for the muon component, the mean-mass temperature of the atmosphere can be used to determine cosmic ray temperature variations.

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