Abundance of nuclei with Z greater than 52 in galactic cosmic rays - Long-term averages based on studies of pallasites

Details Abundance of nuclei with Z greater than 52 in galactic cosmic rays - Long-term averages based on studies of pallasites Abundance of nuclei with Z greater than 52 in galactic cosmic rays - Long-term averages based on studies of pallasites

Nov 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...210..258o&link_type=abstract

Astrophysical Journal, vol. 210, Nov. 15, 1976, pt. 1, p. 258-266.

Astronomy and Astrophysics

Astrophysics

8

Abundance, Cosmic Rays, Heavy Nuclei, Meteoritic Composition, Olivine, Particle Tracks, Calibrating, Fossils, Germanium, Iron, Krypton, Magnetic Flux, Magnetic Poles, Zinc

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1976ApJ...210..258O

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