The Relative Abundances of the Isotopes of Lithium, Beryllium and Boron in the Primary Cosmic Radiation

Details The Relative Abundances of the Isotopes of Lithium, Beryllium and Boron in the Primary Cosmic Radiation The Relative Abundances of the Isotopes of Lithium, Beryllium and Boron in the Primary Cosmic Radiation

Jul 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971ap%26ss..12...98d&link_type=abstract

Astrophysics and Space Science, Volume 12, Issue 1, pp.98-103

Astronomy and Astrophysics

Astrophysics

Scientific paper

Studies have been made to determine the relative abundances of the isotopes of Lithium, Beryllium and Boron in the primary cosmic rays in the low energy interval 180 400 MeV per nucleon recorded in the emulsion stack flown from Fort Churchill. Two independent measurements of mass, wherever possible, were made on each track. Out of nine Boron tracks, 6 particle tracks are consistent with B11 and 3 with B10. Amongst 2 Li tracks, one is consistent with Li6 and the other with Li7.

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