The nitrogen abundance in the cosmic ray source

Details The nitrogen abundance in the cosmic ray source The nitrogen abundance in the cosmic ray source

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9..151w&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 9 (A85-22801 0

Physics

Abundance, Cosmic Rays, Nitrogen Isotopes, Cerenkov Counters, Nuclear Fusion, Oxygen

Scientific paper

In this paper, new cosmic ray data on the isotopic and charge abundance of N nuclei are used, along with new cross section data for the fragmentation of O into N, to re-examine the question of the nitrogen abundance in the cosmic ray source. The cosmic ray data come from balloon flights made in 1976, 1977, and 1978. Both the N-15/N-14 ratio and N/O ratio were measured at the same intermediate energies at which the cross sections were measured, and the N/O ratio was also measured up to about 120 GeV/nuc.

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