All-Union Conference on Cosmic Rays, Dagomys, Russia, Nov. 1-3, 1990, Proceedings

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Conferences, Energetic Particles, Galactic Cosmic Rays, Solar Cosmic Rays, Energy Spectra, Ionospheric Sounding, Magnetohydrodynamic Turbulence, Magnetospheric Instability, Mir Space Station, Nuclear Astrophysics, Particle Acceleration, Plasma-Particle Interactions, Radiation Belts, Radiation Distribution, Solar Cycles, Solar Flares, Solar Protons, Solar Terrestrial Interactions, Solar Wind Velocity

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The present conference on cosmic rays discusses features of the ground-level solar cosmic ray intensity increase on September 28, 1989, from neutron monitor data, large solar proton events at the beginning of the 22nd solar cycle, the solar cosmic ray maximum during the 22nd cycle, and the solar cosmic ray flare in March of 1990. Topics addressed include radiation dynamics along the Mir spacecraft route during the solar proton event of September 29, 1989, accelerated particle dynamics in flare loops, the seasonal behavior of the daily intensities of muons with E not less than 220 GeV, and cosmic ray anisotropy and gradient in different structures of solar wind. Also examined are high-energy electron and positron energy spectra under the earth's radiation belt, Galactic cosmic ray intensity during the beginning of the sun's global magnetic field reversal, the propagation of cosmic rays in the magnetic field with large-scale inhomogeneities, and north-south asymmetry of the nonperiodic and quasi-periodic cosmic ray variations.

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