Quasi-quinquennial variation in cosmic ray intensity

Details Quasi-quinquennial variation in cosmic ray intensity Quasi-quinquennial variation in cosmic ray intensity

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...10...47o&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 10 (A85-22801

Physics

Annual Variations, Galactic Cosmic Rays, Particle Flux Density, Solar Activity Effects, Interplanetary Magnetic Fields, Magnetic Variations, Power Spectra

Scientific paper

Clear evidence for the existence of a quasi-quinquennial variation in cosmic ray intensity is shown by an analysis of monthly averages of the neutron monitor intensity observed at various observatories over the period 1958 - 1980. The variation is well correlated with a corresponding variation in solar activity. It is suggested that a small change in the heliospheric boundary location of approximately 0.7 AU could produce this variation.

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