Quasistationary asymmetry of the galactic cosmic ray density distribution in the heliosphere.

Details Quasistationary asymmetry of the galactic cosmic ray density distribution in the heliosphere. Quasistationary asymmetry of the galactic cosmic ray density distribution in the heliosphere.

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...10...71u&link_type=abstract

18th International Cosmic Ray Conference, Vol. 10, p. 71 - 74

Physics

Cosmic Rays:Density Distribution, Cosmic Rays:Meteorites, Cosmic Rays:Solar Modulation, Meteorites:Cosmic Rays

Scientific paper

The results of the investigation of cosmogenic radionuclides in meteorites evidence that the 11-year periods of the maximum north-south asymmetry in the galactic cosmic ray density distribution in the heliosphere are replaced by the 11-year periods of the minimum one, and, on the average over a million years some residual asymmetry, apparently, exists.

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