Integral multiplicities of the general ionizing component of cosmic rays at different depths of the earth atmosphere

Details Integral multiplicities of the general ionizing component of cosmic rays at different depths of the earth atmosphere Integral multiplicities of the general ionizing component of cosmic rays at different depths of the earth atmosphere

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55.1992a&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, Russia, Nov. 1-3, 1990, Materialy. A92-40776 16-93) Akademiia Nauk

Computer Science

Atmospheric Effects, Earth Atmosphere, Galactic Cosmic Rays, Ionizing Radiation, Particle Flux Density, Energetic Particles, Monte Carlo Method

Scientific paper

The Monte Carlo method is used to calculate coupling coefficients for the general ionizing component of cosmic rays at different depths in the atmosphere. These coefficients are employed to evaluate the intensity of the cosmic ray ionizing component in the solar minima of 1965, 1976, and 1987. It is concluded that significant residual modulation in the high-energy region took place in the 1976 solar minimum.

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