Simulation of long-term cosmic-ray intensity variation

Details Simulation of long-term cosmic-ray intensity variation Simulation of long-term cosmic-ray intensity variation

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..125..409m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 125, Feb. 1990, p. 409-414.

Physics

9

Galactic Cosmic Rays, Solar Cycles, Earth Magnetosphere, Geomagnetism, Intensity, Magnetic Rigidity, Radiant Flux Density, Simulation

Scientific paper

An attempt is made to reproduce to a certain degree the long-term modulation of Galactic cosmic rays using monthly cosmic-ray data from nine worldwide neutron monitor stations for the period 1975-1985. The empirical formula which is used to compute the long-term cosmic-ray variations follows the observations fairly well. It is noteworthy that the residuals in the cosmic-ray intensity between that observed and that calculated by this empirical formula exhibits a still-remaining, short-term variation in all stations of 2.7 and 3.7 months. Possible interpretations of these observed periodicities related to Galactic origin are given.

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