The response of the middle atmosphere to the effects of galactic cosmic rays.

Details The response of the middle atmosphere to the effects of galactic cosmic rays. The response of the middle atmosphere to the effects of galactic cosmic rays.

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..500v&link_type=abstract

Geomagn. Aeron., Vol. 30, No. 4, p. 500 - 504

Computer Science

Cosmic Rays: Earth Atmosphere

Scientific paper

An improved model is devised for the interaction of cosmic rays with the middle atmosphere. Profiles of the ionization q(h) are calculated as a function of the composition (protons, α particles, L, M, H, and VH groups of the nucleus) and energy spectrum of the penetrating high-energy particles. A computer program is set up to realize the Gauss algorithm for the solution of multiple integrals. The q(h) profiles are plotted in the 25 - 80 km range, together with the N(h) profiles of the 50 - 80 km layer for periods of maximum and minimum solar activity.

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