Time variation of galactic cosmic rays

Details Time variation of galactic cosmic rays Time variation of galactic cosmic rays

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ippe.conf..149e&link_type=abstract

In Jet Propulsion Lab., California Inst. of Tech., Interplanetary Particle Environment. Proceedings of a Conference p 149-161 (S

Mathematics

Logic

Galactic Cosmic Rays, Solar Cycles, Solar Flares, Sun, Time, Variations, Current Sheets, Mathematical Models

Scientific paper

Time variations in the flux of galactic cosmic rays are the result of changing conditions in the solar wind. Maximum cosmic ray fluxes, which occur when solar activity is at a minimum, are well defined. Reductions from this maximum level are typically systematic and predictable but on occasion are rapid and unexpected. Models relating the flux level at lower energy to that at neutron monitor energy are typically accurate to 20 percent of the total excursion at that energy. Other models, relating flux to observables such as sunspot number, flare frequency, and current sheet tilt are phenomenological but nevertheless can be quite accurate.

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