An intricate course of intensity growth in solar cosmic rays with intensities of 1-20 and more than 20 MeV has been analyzed. The event was caused by a sequence of six intense solar flares occurring in the same active region at solar latitudes from E65 to W69. This fact has determined an important role of the solar latitude effect on the propagation of solar cosmic rays and flare disturbances. The use of the "reflection" model has revealed the influence of solar flares on the modulation of solar cosmic and galactic cosmic ray streams.
Research Institute of Nuclear Physics, Faculty of Physics, Moscow State University, Leninskie Gory, Moscow, 119992, Russia
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