Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Cosmic ray isotope abundances from chromium to nickel

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/157119· OSTI ID:6094550
IRIS, a telescope consisting of a large-area, precision Cerenkov detector, scintillators, spark chambers, and a passive stack of Lexan polycarbonate track detectors, was exposed to the primary cosmic radiation for 6.6 m/sup 2/ sr hr in a balloon flight in 1976. This measurement has yielded the isotopic composition of the iron-group elements Cr, Mn, Fe, and Ni with an average mass resolution of 0.65 amu for the energies 320--500 MeV per amu at the detector. This experiment places the most severe constraints to date on deviation from solar system composition of the source of the cosmic radiation. We place upper limits of 10% on the ratios /sup 54/Fe//sup 56/Fe and /sup 58/Fe//sup 56/Fe, which are inconsistent with large departures from solar system source composition reported by other workers. The isotopic measurements of Fe and Ni preclude the possibility that these cosmic rays were produced in a single e-process zone. The mean mass of Mn is lesss than 55, indicating the presence of electron capture species produced by spallation.
Research Organization:
Department of Physics, University of California, Berkeley
OSTI ID:
6094550
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 230:2; ISSN ASJOA
Country of Publication:
United States
Language:
English