Sub-iron to iron nuclei in low-energy (50-200 MeV/nucl) cosmic rays as observed in the SKYLAB experiment

Details Sub-iron to iron nuclei in low-energy (50-200 MeV/nucl) cosmic rays as observed in the SKYLAB experiment Sub-iron to iron nuclei in low-energy (50-200 MeV/nucl) cosmic rays as observed in the SKYLAB experiment

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.149..163d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 149, no. 1, Nov. 1988, p. 163-170.

Astronomy and Astrophysics

Astrophysics

5

Cosmic Rays, Cosmochemistry, Iron, Nuclear Astrophysics, Spaceborne Experiments, Abundance, Particle Energy, Skylab Program, Spectral Energy Distribution

Scientific paper

The authors present their most recent results on the sub-iron (Sc to Cr) to Fe nuclei abundance ratios in the low-energy cosmic rays of 50 to 250 MeV nucl.-1 and their implications as observed in the Skylab experiment. In view of the importance of this ratio in determining the cosmic-ray pathlength in interstellar medium, the authors have obtained additional data in the same detector module and the results of final analysis are reported.

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