Model description of differential galactic-cosmic-ray spectra

Details Model description of differential galactic-cosmic-ray spectra Model description of differential galactic-cosmic-ray spectra

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978izyak..42..923k&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, June 1977.) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheska

Physics

Nuclear Physics

Cosmic Rays, Energy Spectra, Galactic Radiation, Particle Flux Density, Solar Activity Effects, Solar Cycles, Alpha Particles, Correlation Coefficients, Modulation, Nuclei (Nuclear Physics), Proton Flux Density

Scientific paper

The differential spectra of protons, alpha particles, and other galactic-cosmic-ray charge groups are modeled as a function of phase of solar activity cycle. The relation between parameters of proton and alpha-particle modulation and mean yearly Wolf numbers is investigated. Correlation coefficients are computed for several different years in a solar activity cycle.

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