Behavior of solar activity and cosmic rays during the 19th and 20th cycles

Details Behavior of solar activity and cosmic rays during the 19th and 20th cycles Behavior of solar activity and cosmic rays during the 19th and 20th cycles

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979izyer..43.2599l&link_type=abstract

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

Computer Science

Cosmic Rays, Galactic Radiation, Solar Activity Effects, Solar Cycles, Phase Diagrams, Radiant Flux Density

Scientific paper

Kontor et al. (1978) showed that variations with a period of 25 months were present during the 20th cycle of solar activity, in particular at its descent phase. Analogous, but antiphase, variations were observed for the intensity of galactic cosmic rays of various energies. In the present paper, fairly smooth curves of the 11-year component are obtained by applying the moving average method to the initial (three-month) data. The characteristic features of this curve are compared to those of the solar activity curve for the period from 1953 to 1977.

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