Concerning the 22-year cycle of galactic cosmic ray intensity

Details Concerning the 22-year cycle of galactic cosmic ray intensity Concerning the 22-year cycle of galactic cosmic ray intensity

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979izyer..43.2603k&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yerevan, Armenian SSR, June 1979.) Akademiia Nauk SSSR, Izvestiia, Seriia Fi

Physics

Cosmic Rays, Galactic Radiation, Particle Flux Density, Charged Particles, Cycles, Interplanetary Magnetic Fields, Photosphere, Polar Regions, Solar Magnetic Field

Scientific paper

The paper examines the features of galactic cosmic rays before and after the 1969-1971 period, which was characterized by an inversion of the high-latitude magnetic field of the photosphere. Various theoretical interpretations of the relationship between cosmic ray characteristics and solar magnetic field polarity are discussed. It is suggested that this relationship is determined by particle gradient drift, whose direction depends on the sign of regular interplanetary magnetic fields and on the sign of particle charge. This interpretation provides a good explanation for the observed 22-year cycle of galactic cosmic ray intensity.

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