Galactic cosmic ray variations in the heliosphere according to radioactivity of meteorites

Details Galactic cosmic ray variations in the heliosphere according to radioactivity of meteorites Galactic cosmic ray variations in the heliosphere according to radioactivity of meteorites

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...10...42a&link_type=abstract

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

Computer Science

Galactic Cosmic Rays, Heliosphere, Meteoritic Composition, Particle Flux Density, Radioactive Isotopes, Chondrites, Modulation, Solar Activity Effects

Scientific paper

The results of the investigation of cosmogenic radionuclides in meteorites testify to the fact that the galactic cosmic ray (GCR) modulation range in the heliosphere is not spherical, but is compressed in the meridional plane, mainly, within the heliolatitudinal region of + or - 40 deg. It has, apparently, a fine structure with the maximum GCR gradients at + or (10-25) deg. Such a form of the modulation range has existed at least over a million years being, however, on the average, somewhat more stretched southward from the helioequator.

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