Investigation of weight relationships of different mechanisms of cosmic-ray anisotropy

Details Investigation of weight relationships of different mechanisms of cosmic-ray anisotropy Investigation of weight relationships of different mechanisms of cosmic-ray anisotropy

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2438g&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser

Physics

Anisotropic Media, Diffusion Theory, Galactic Cosmic Rays, Interplanetary Space, Dynamic Characteristics, Interplanetary Magnetic Fields, Periodic Variations, Solar Wind

Scientific paper

It is shown that the weight contribution of the antisymmetric diurnal variation to the average annual first harmonic of the angular distribution of galactic cosmic rays is negligibly small. The main mechanism responsible for the observed anisotropy is a convective-diffusive one, taking the adiabatic deceleration of particles into account. The energy spectrum of this mechanism does not change with the solar cycle.

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