Long-period variations of cosmic-ray anisotropy

Details Long-period variations of cosmic-ray anisotropy Long-period variations of cosmic-ray anisotropy

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2129k&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Computer Science

Anisotropy, Cosmic Rays, Interplanetary Magnetic Fields, Particle Flux Density, Periodic Variations, Solar Activity Effects, Annual Variations, Diurnal Variations, Heliosphere, Muons, Particle Diffusion, Solar Wind Velocity

Scientific paper

The diurnal-variation characteristics of cosmic-ray intensity are investigated on the basis of muon data for 1937-1983. Eleven-year and 22-year variations of cosmic-ray anisotropy are observed which are due to anisotropic diffusion. It is shown that, in the case of an open heliosphere, an additional diffusional outflow of particles from the heliosphere in the ecliptic plane can be produced, which compensates for the increase of wind velocity at high latitudes.

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