Preliminary results from measurements in nuclear emulsions of the isotopic composition of cosmic-ray nitrogen and oxygen
Technical Report
·
OSTI ID:7312418
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 /sup 16/O nuclei with a small fraction of heavier nuclei. /sup -14/N seems to be more abundant than /sup -15/N. (GRA)
- Research Organization:
- Lund Univ. (Sweden)
- OSTI ID:
- 7312418
- Report Number(s):
- N-75-33994; LUIP-CR-74-17
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640101* -- Astrophysics & Cosmology-- Cosmic Radiation
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CHEMICAL COMPOSITION
COSMIC RADIATION
ENERGY RANGE
GEV RANGE
GEV RANGE 01-10
IONIZING RADIATIONS
ISOTOPE RATIO
MASS SPECTRA
NITROGEN ISOTOPES
NUCLEAR EMULSIONS
OXYGEN ISOTOPES
PARTICLE TRACKS
RADIATIONS
SPECTRA
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CHEMICAL COMPOSITION
COSMIC RADIATION
ENERGY RANGE
GEV RANGE
GEV RANGE 01-10
IONIZING RADIATIONS
ISOTOPE RATIO
MASS SPECTRA
NITROGEN ISOTOPES
NUCLEAR EMULSIONS
OXYGEN ISOTOPES
PARTICLE TRACKS
RADIATIONS
SPECTRA