Secondary components, integral multiplicities, and coupling coefficients of cosmic rays in the atmospheres of the earth and other planets

Details Secondary components, integral multiplicities, and coupling coefficients of cosmic rays in the atmospheres of the earth and other planets Secondary components, integral multiplicities, and coupling coefficients of cosmic rays in the atmospheres of the earth and other planets

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979izyer..43.2628d&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yerevan, Armenian SSR, June 1979.) Akademiia Nauk SSSR, Izvestiia, Seriia Fi

Computer Science

Coupling Coefficients, Earth Atmosphere, Planetary Atmospheres, Secondary Cosmic Rays, Electron Flux Density, Hadrons, Kinetic Equations, Muons, Numerical Integration

Scientific paper

Integral multiplicities of cosmic ray production are calculated on the
basis of kinetic equations describing hadron cascades in the atmosphere.
The multiplicities are then used to obtain coupling coefficients for the
nucleon, muon, and electron components of secondary cosmic rays.

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