Preliminary results from measurements in nuclear emulsions of the isotopic composition of cosmic ray nitrogen and oxygen

Details Preliminary results from measurements in nuclear emulsions of the isotopic composition of cosmic ray nitrogen and oxygen Preliminary results from measurements in nuclear emulsions of the isotopic composition of cosmic ray nitrogen and oxygen

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974stin...7533994j&link_type=abstract

Presented at the Symp. on Meas. and Interpretation of the Isotopic Composition of Solar and Galactic Cosmic Rays, Durham, N. H.,

Computer Science

Cosmic Rays, Nitrogen Isotopes, Nuclear Emulsions, Oxygen Isotopes, Abundance, Balloon Flight, Canada, Mass Spectra, Particle Tracks

Scientific paper

Determination of isotopic masses of nitrogen and oxygen were made in a small stack of nuclear emulsion exposed in a balloon flight from Fort Churchill, Canada, in June 1970, from relations between track width and residual range. The mass spectra are the spectra of stopping nuclei, and their mean energy falls in the range 200 to 400 MeV/nucleon. The main peak for oxygen consists of 0.16 nuclei with a small fraction of heavier nuclei. N-14 seems to be more abundant than N-15.

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