The Relative Abundances of the Isotopes of Light Nuclei (Li, Be and B) in the Primary Cosmic Radiation

Details The Relative Abundances of the Isotopes of Light Nuclei (Li, Be and B) in the Primary Cosmic Radiation The Relative Abundances of the Isotopes of Light Nuclei (Li, Be and B) in the Primary Cosmic Radiation

Jul 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971ap%26ss..12..243d&link_type=abstract

Astrophysics and Space Science, Volume 12, Issue 1, pp.243-249

Astronomy and Astrophysics

Astrophysics

Scientific paper

Studies have been made to determine the relative abundances of the isotopes of Lithium and Boron in the primary cosmic rays in the low energy interval 120 400 MeV per nucleon recorded in the emulsion stack flown from Fort Churchill. Two independent measurements of mass, wherever possible, were made on each track by the range vs ionisation method. The results obtained on nine stopping Boron nuclei and two Lithium nuclei are presented.

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