Physics
Scientific paper
Apr 1967
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967jatp...29..385d&link_type=abstract
Journal of Atmospheric and Terrestrial Physics, vol. 29, no. 4, pp. 385-394
Physics
Scientific paper
The dependence of the solar cosmic ray diffusion coefficient upon the cosmic ray energy and distance to the Sun has been studied. The magnetic field strength in the inhomogeneities, their dimensions and distances between them have been evaluated. The spectrum of the solar particle generation in the energy range 1-1000 MeV has been obtained for the flare on September 28, 1961. The influence of the duration of the solar cosmic ray ejection from the acceleration region on the cosmic ray spatial distribution in the interplanetary space is discussed. The multiplicities of the generation of the neutron and hard component in the Earth's atmosphere have been calculated. The rigidity spectrum for the 1-15 BV range has been obtained at the atmospheric boundary for the particles from the flare on February 23, 1956. An attempt is made to explain some features of the energy spectrum of the solar cosmic rays taking account of the combined dependence of the diffusion coefficient upon the particle energies and distance to the Sun. The geo-effectiveness of the solar cosmic ray bursts on September 28, 1961 and July 14-15, 1959 has been evaluated.
Dorman Lev I.
Miroshnichenko Leonty I.
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