On the Energy Dependence of the Ratio of Li, Be and B to C, N, O and F Nuclei in the Primary Cosmic Rays

Details On the Energy Dependence of the Ratio of Li, Be and B to C, N, O and F Nuclei in the Primary Cosmic Rays On the Energy Dependence of the Ratio of Li, Be and B to C, N, O and F Nuclei in the Primary Cosmic Rays

Sep 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969ap%26ss...5...59b&link_type=abstract

Astrophysics and Space Science, Volume 5, Issue 1, pp.59-67

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

A critical study of all available data on the energy dependence of the ratio ff the intensities of Li, Be, and B to C, N, O and F nuclei (L/M-ratio) in cosmic rays is made. It seems that in a recent experiment by Von Rosenvingeet al. (1969), the flux of M-nuclei has come out higher in the energy interval of 200 400 MeV/nucleon and that of L-nuclei lower in the energy interval 400 600 MeV/nucleon; as a result they obtained a value of the ratio of L/M which is about 50% lower than all other investigators. The results of all other studies yield the best estimate of the ratio of L/M as 0.26±0.03, 0.41±0.03 and 0.26±0.02 in the energy interval 50 150, 200 600 and>1500 MeV/nucleon respectively.

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