Eleven-year cosmic-ray cycle in the stratosphere

Details Eleven-year cosmic-ray cycle in the stratosphere Eleven-year cosmic-ray cycle in the stratosphere

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ge%26ae..18..385c&link_type=abstract

(Geomagnetizm i Aeronomiia, vol. 18, May-June 1978, p. 385-405.) Geomagnetism and Aeronomy, vol. 18, Dec. 1978, p. 259-271. Tra

Physics

Cosmic Rays, Particle Flux Density, Solar Activity Effects, Solar Cycles, Solar Terrestrial Interactions, Stratosphere, Energy Spectra, Numerical Integration, Secular Variations, Solar Flux, Sunspots

Scientific paper

In the present paper, an attempt is made to elucidate the principal features of the large-scale cosmic ray variations, caused by the 11-year cycle of solar activity, on the basis of a review of contemporary theoretical and experimental data. The discussion covers such topics as the time dependences of cosmic ray intensity in the stratosphere; the relationship between cosmic ray intensity and solar-activity parameters; and the relationship between the 11-year cosmic ray modulation coefficient and the particle energy spectrum. The analysis points toward a much smaller 11-year cycle modulation region (10 to 20 AU) than formerly assumed.

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