Seasonal and diurnal variations of cosmic-ray intensity according to measurement at a depth of about 8.5 x 10 to the 4th g/sq cm

Details Seasonal and diurnal variations of cosmic-ray intensity according to measurement at a depth of about 8.5 x 10 to the 4th g/sq cm Seasonal and diurnal variations of cosmic-ray intensity according to measurement at a depth of about 8.5 x 10 to the 4th g/sq cm

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2432a&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser

Computer Science

Annual Variations, Cosmic Rays, Earth Atmosphere, Radiant Flux Density, Atmospheric Boundary Layer, Atmospheric Temperature, Upper Atmosphere

Scientific paper

Baksan scintillation-counter measurements for a period extending from
January 1, 1983 to December 31, 1987 are analyzed. It is shown that
seasonal variations of the intensity of the cosmic-ray muon component at
energies not less than 220 GeV are caused by thermal processes in the
upper layers of the atmosphere.

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