Galactic Cosmic-Ray Distributions in the Heliosphere During Four Solar Cycles as Evidenced by Radionuclides in Successively Fallen Chondrites

Details Galactic Cosmic-Ray Distributions in the Heliosphere During Four Solar Cycles as Evidenced by Radionuclides in Successively Fallen Chondrites Galactic Cosmic-Ray Distributions in the Heliosphere During Four Solar Cycles as Evidenced by Radionuclides in Successively Fallen Chondrites

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1076u&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1076

Physics

1

Scientific paper

A picture of variation of the galactic cosmic ray integral gradients in
1955-1992 along the orbits of 14 freshfallen chondrites is presented.
Some peculiarities of electromagnetic structure of the heliosphere are
derived.

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