Dependence of the propagation of ultra-heavy cosmic ray nuclei on first ionization potential.

Details Dependence of the propagation of ultra-heavy cosmic ray nuclei on first ionization potential. Dependence of the propagation of ultra-heavy cosmic ray nuclei on first ionization potential.

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998acppb..29..357f&link_type=abstract

Acta Phys. Pol., B, Vol. 29, No. 1 - 2, p. 357 - 363

Physics

Cosmic Rays: Ultrahigh Energy

Scientific paper

Over 2000 ultra heavy (Z ≥ 65) cosmic ray ions with energies over 3 GeV/n have been recorded in the UHCRE, of which a total of 205 have already been located, measured and positively identified as ultra heavy (UH) ions. A histogram of UH elemental abundances in the Earth's neighbourhood is obtained and UH cosmic ray source abundances may be determined by means of an appropriate propagation model. This model describes the travel of UH ions from their sources to near the Earth, through the interstellar medium.

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