Determination of the ionization by cosmic rays during daytime

Details Determination of the ionization by cosmic rays during daytime Determination of the ionization by cosmic rays during daytime

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...10..270k&link_type=abstract

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

Physics

Atmospheric Ionization, Cosmic Rays, Solar Terrestrial Interactions, Angles (Geometry), Daytime, Flux Quantization, Solar Position, Zenith

Scientific paper

Two methods are presented for determining the ionization due to cosmic rays in the atmosphere. The first method is based on the fact that the latitudinal dependence of cosmic ray flux is different from that of solar electromagnetic radiation (cosmic ray intensity increases with latitude, while solar radiation flux decreases). The second method makes use of the fact that, unlike solar energy flux, cosmic ray flux is independent of the zenith angle. Both methods are illustrated by examples.

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