Investigation of the modulation of galactic cosmic rays

Details Investigation of the modulation of galactic cosmic rays Investigation of the modulation of galactic cosmic rays

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981izssr..45.1287a&link_type=abstract

(Evropeiskii Simpozium po Kosmicheskim Lucham, 7th, Leningrad, USSR, Sept. 15-19, 1980.) Akademiia Nauk SSSR, Izvestiia, Seriia

Astronomy and Astrophysics

Astronomy

Cosmic Rays, Galactic Radiation, Interplanetary Space, Periodic Variations, Solar Activity Effects, Astronomical Models, Convective Flow, Data Reduction, Energy Spectra, Modulation, Particle Diffusion, Particle Intensity

Scientific paper

A unified convection-diffusion model for the propagation of galactic cosmic rays in interplanetary space is used to study different variations of cosmic rays, from semidiurnal to 11-year. An analysis is presented of physical data concerning these variations: the effective dimensions of the modulation region; the residual modulation during the solar activity minima of 1954, 1965, and 1976; and radial and transverse gradients of cosmic-ray intensity. Energy spectra for these variations are obtained.

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