Computer Science
Scientific paper
Sep 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974izssr..38.1920d&link_type=abstract
(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Kharkov, Ukrainian SSR, Sept. 25-28, 1973.) Akademiia Nauk SSSR, Izv
Computer Science
Cosmic Rays, Galactic Radiation, Interplanetary Space, Radiation Distribution, Solar Activity Effects, Solar Cosmic Rays, Anisotropy, Isotropy, Particle Flux Density, Solar Wind, Spatial Distribution, Sunspots
Scientific paper
An attempt is made to check and to define more precisely the HL-index of solar activity on the basis of a comparison with analytical calculations of the spatial distribution of cosmic rays in interplanetary space, using a model which combines both anisotropic (at distances of 2 to 3 AU from the sun) and isotropic (at large distances) diffusion of cosmic rays. The forms of the HL-index which provide the best description of the modulation depth for various distances from the sun and various heliolatitudes of the point of observation are identified.
Dorman Lev I.
Gushchina R. T.
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