Physics
Scientific paper
Feb 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ssrv...34..127a&link_type=abstract
(COSPAR, IAU, IUGG, IUPAP, and URSI, International Symposium on Progress in Solar-Terrestrial Physics, 5th, Ottawa, Canada, May
Physics
13
Cosmic Rays, Galactic Radiation, Heliosphere, Particle Flux Density, Solar Cosmic Rays, Solar Cycles, Interplanetary Magnetic Fields, Neutrons, Secular Variations, Solar Wind, Sunspots
Scientific paper
Results recently obtained for cosmic ray intensities at energies greater than 1 GeV, by means of ground-based detectors, are discussed with attention to long-term changes in the isotropic and anisotropic cosmic ray intensity components. Significant changes in cosmic ray modulation noted in the 1969-1970 period are related to solar poloidal field reversal, and their characteristics are described in order to relate them to the heliospheric configuration. Detailed consideration is given to variational characteristic anomalies for both the isotropic and the anisotropic parts of cosmic ray intensity. Phenomena with 11- and 22-year periodicities are found to occur simultaneously, and their derived relative importance is related to interplanetary variables.
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