Temporal, radial, and latitudinal variations of galactic cosmic ray gradients in the solar system

Details Temporal, radial, and latitudinal variations of galactic cosmic ray gradients in the solar system Temporal, radial, and latitudinal variations of galactic cosmic ray gradients in the solar system

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981izssr..45..547l&link_type=abstract

(Evropeiskii Simpozium po Kosmicheskim Lucham, 7th, Leningrad, USSR, Sept. 15-19, 1980.) Akademiia Nauk SSSR, Izvestiia, Seriia

Computer Science

Cosmic Rays, Galactic Radiation, Gradients, Periodic Variations, Solar System, Spatial Dependencies, Ecliptic, Meteoritic Composition, Solar Activity Effects, Solar Wind

Scientific paper

An analysis of the radioactivity of stony meteorites has made it possible to obtain information on galactic cosmic ray gradients during the period 1955-1976, as well as their mean values for one-million years at heliocentric distances of 1.03-3.33 AU and solar latitudes from 23.1 S and 15.7 N. The dependence of radial and transverse gradients on the phase of the solar cycle is investigated.

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