Correlation of source abundances of ultraheavy cosmic rays with first ionization potential - Results from HEAO-3

Details Correlation of source abundances of ultraheavy cosmic rays with first ionization potential - Results from HEAO-3 Correlation of source abundances of ultraheavy cosmic rays with first ionization potential - Results from HEAO-3

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9..305i&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 9 (A85-22801 0

Computer Science

Abundance, Cosmic Rays, Heao 3, Heavy Nuclei, Correlation, Germanium, Ionization Potentials, Iron, Magnesium, Nickel, Silicon, Solar System

Scientific paper

The HEAO-3 heavy nuclei experiment yields the abundances of many individual elements of even atomic number (Z) in the interval 26 ≤ Z ≤ 58. The cosmic-ray-source (CRS) abundances, which have been derived from these observations using standard propagation models is compared with solar-system (SS) abundances. The correlation of the CRS/SS ratio with first ionization potential is presented.

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