Response of the middle atmosphere to Galactic cosmic rays

Details Response of the middle atmosphere to Galactic cosmic rays Response of the middle atmosphere to Galactic cosmic rays

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..593v&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 30, July-Aug. 1990, p. 593-598. In Russian.

Computer Science

4

Atmospheric Ionization, Galactic Cosmic Rays, Middle Atmosphere, Computer Programs, Energetic Particles, Energy Spectra

Scientific paper

An improved model describing the interaction of cosmic rays with the middle atmosphere is developed. Ionization profiles q(h) are calculated as a function of the composition (protons, alpha particles, and the L, M, H, and VH groups of nuclei) and the energy spectrum of penetrating high-energy particles. A computer program implementing the Gauss algorithm for the solution of multiple integrals has been devised. Ionization profiles in the 25-80 height range and N(h) profiles in the 50-80 region were obtained for the solar maximum and minimum periods.

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